This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76
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 05 03.2894 2461163.7894 10.21 19:40:03.67 +34:40:51.0
68.99252 6.04714 galactic Cyg Second-epoch detections are separated by 1.4" and 4.5 pix
The object was found in VSX 6" ZTF J194004.13+344054.1
Type: SR
# Max. Min./Amp. JD0 Period
13.010 g Y 0.354 g 2458439.30320 255.795359700000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:40:03.67 +34:40:51.0: 11.31 +/- 0.01 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:40:03.67 +34:40:51.0: 11.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 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
ZTF J194004.13+344054.1,2461163.7894,10.21,0.05,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
ZTF J194004.13+344054.1 20260503.2894 10.21CV 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 05 03.2894 2461163.7894 12.29 19:47:27.71 +25:55:01.4
62.15779 0.31868 galactic Vul Second-epoch detections are separated by 8.4" and 3.3 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 J296.8591+25.9128 | 19:47:28.45 +25:54:49.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:47:27.71 +25:55:01.4: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:47:27.71 +25:55:01.4: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.8591+25.9128,2461163.7894,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.8591+25.9128 20260503.2894 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 05 03.2894 2461163.7894 12.15 19:41:36.32 +35:19:38.5
69.71531 6.08451 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 | ATO J295.4022+35.3177 | 19:41:36.94 +35:19:29.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:41:36.32 +35:19:38.5: 14.36 +/- 0.17 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:41:36.32 +35:19:38.5: 12.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.4022+35.3177,2461163.7894,12.15,0.05,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 J295.4022+35.3177 20260503.2894 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 05 03.2894 2461163.7894 11.99 19:50:23.29 +33:14:52.5
68.80818 3.47737 galactic Cyg Second-epoch detections are separated by 3.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2034764469030808320 | 19:50:21.51 +33:15:14.3 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:50:23.29 +33:14:52.5: 13.19 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:50:23.29 +33:14:52.5: 13.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2034764469030808320,2461163.7894,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034764469030808320 20260503.2894 11.99CV 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 05 03.2894 2461163.7894 12.02 20:02:49.55 +33:54:12.0
70.71379 1.60217 galactic Cyg Second-epoch detections are separated by 5.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.6974+33.9004 | 20:02:48.77 +33:54:07.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.907+/- (M)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:02:49.55 +33:54:12.0: 12.96 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:02:49.55 +33:54:12.0: 12.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.6974+33.9004,2461163.7894,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.6974+33.9004 20260503.2894 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.91 20:04:48.78 +33:58:38.5
70.99612 1.29284 galactic Cyg Second-epoch detections are separated by 3.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2058360538302798720 | 20:04:49.11 +33:58:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:04:48.78 +33:58:38.5: 13.46 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:04:48.78 +33:58:38.5: 13.70 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 2058360538302798720,2461163.7894,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2058360538302798720 20260503.2894 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.77 19:44:44.31 +34:09:27.2
69.00827 4.94986 galactic Cyg Second-epoch detections are separated by 4.8" and 4.4 pix
The object was found in VSX23" HAT 199-01319
Type: LPV
# Max. Min./Amp. JD0 Period
9.127 Ic 9.182 Ic
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:44:44.31 +34:09:27.2: 13.06 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:44:44.31 +34:09:27.2: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-01319,2461163.7894,11.77,0.05,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
HAT 199-01319 20260503.2894 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 05 03.2894 2461163.7894 11.83 19:55:54.94 +31:58:00.4
68.30359 1.82142 galactic Cyg Second-epoch detections are separated by 3.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J298.9720+31.9712 | 19:55:53.30 +31:58:16.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:55:54.94 +31:58:00.4: 13.22 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:55:54.94 +31:58:00.4: 13.35 +/- 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 J298.9720+31.9712,2461163.7894,11.83,0.05,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 J298.9720+31.9712 20260503.2894 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 05 03.2894 2461163.7894 11.67 20:03:02.35 +33:26:28.1
70.34562 1.31909 galactic Cyg Second-epoch detections are separated by 3.1" 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 2058225916868762752 | 20:02:59.63 +33:26:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:03:02.35 +33:26:28.1: 13.46 +/- 0.07 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:03:02.35 +33:26:28.1: 13.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2058225916868762752,2461163.7894,11.67,0.05,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
Gaia DR3 2058225916868762752 20260503.2894 11.67CV 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 05 03.2894 2461163.7894 11.51 19:59:27.48 +33:21:28.5
69.88024 1.91000 galactic Cyg Second-epoch detections are separated by 1.9" and 4.7 pix
The object was found in VSX19" Gaia DR3 2034402248681279616
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.250 G 11.280 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:59:27.48 +33:21:28.5: 13.12 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:59:27.48 +33:21:28.5: 12.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034402248681279616,2461163.7894,11.51,0.05,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 2034402248681279616 20260503.2894 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 05 03.2894 2461163.7894 10.78 20:00:27.78 +32:42:36.0
69.43943 1.39037 galactic Cyg Second-epoch detections are separated by 5.5" and 4.6 pix
The object was found in VSX20" Gaia DR3 2034158844283093376
Type: E
# Max. Min./Amp. JD0 Period
17.490 G 17.690 G 7.745400000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:00:27.78 +32:42:36.0: 12.21 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:00:27.78 +32:42:36.0: 12.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034158844283093376,2461163.7894,10.78,0.05,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 2034158844283093376 20260503.2894 10.78CV 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 05 03.2894 2461163.7894 10.99 19:33:29.89 +31:31:18.1
65.54334 5.73609 galactic Cyg Second-epoch detections are separated by 1.0" and 4.8 pix
The object was found in VSX16" Gaia DR3 2044836407856380288
Type: RS
# Max. Min./Amp. JD0 Period
16.870 G 16.940 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:33:29.89 +31:31:18.1: 12.75 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:33:29.89 +31:31:18.1: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2044836407856380288,2461163.7894,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2044836407856380288 20260503.2894 10.99CV 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 05 03.2894 2461163.7894 11.06 20:10:43.28 +34:52:50.1
72.41489 0.75636 galactic Cyg Second-epoch detections are separated by 6.4" and 3.6 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 | ASASSN-V J201040.50+345245.9 | 20:10:40.49 +34:52:45.9 (Gaia DR3) | SR (local) | 24.851103000000 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:10:43.28 +34:52:50.1: 12.77 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:10:43.28 +34:52:50.1: 13.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201040.50+345245.9,2461163.7894,11.06,0.05,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
ASASSN-V J201040.50+345245.9 20260503.2894 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 05 03.2894 2461163.7894 11.19 19:37:51.32 +32:24:52.5
66.77573 5.35328 galactic Cyg Second-epoch detections are separated by 4.6" and 3.9 pix
The object was found in VSX23" Gaia DR3 2045357404567351808
Type: ROT
# Max. Min./Amp. JD0 Period
16.730 G 16.790 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:37:51.32 +32:24:52.5: 12.44 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:37:51.32 +32:24:52.5: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2045357404567351808,2461163.7894,11.19,0.05,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
Gaia DR3 2045357404567351808 20260503.2894 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 05 03.2894 2461163.7894 11.14 20:00:21.27 +33:16:03.9
69.90188 1.70326 galactic Cyg Second-epoch detections are separated by 2.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0984+33.2667 | 20:00:23.62 +33:16:00.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:00:21.27 +33:16:03.9: 13.38 +/- 0.07 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:00:21.27 +33:16:03.9: 13.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 J300.0984+33.2667,2461163.7894,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0984+33.2667 20260503.2894 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.24 20:02:32.03 +32:08:41.0
69.19053 0.72063 galactic Cyg Second-epoch detections are separated by 3.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2031080039923961728 | 20:02:32.52 +32:09:12.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:02:32.03 +32:08:41.0: 13.26 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:02:32.03 +32:08:41.0: 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 2031080039923961728,2461163.7894,11.24,0.05,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 2031080039923961728 20260503.2894 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 05 03.2894 2461163.7894 11.37 20:15:52.48 +30:07:55.9
69.05268 -2.76908 galactic Cyg Second-epoch detections are separated by 1.9" 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 1861495523966982400 | 20:15:54.73 +30:07:59.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:15:52.48 +30:07:55.9: 12.86 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:15:52.48 +30:07:55.9: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1861495523966982400,2461163.7894,11.37,0.05,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 1861495523966982400 20260503.2894 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 05 03.2894 2461163.7894 11.23 19:30:08.69 +34:48:09.9
68.12732 7.89838 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 | Gaia DR3 2046775495361598208 | 19:30:10.21 +34:48:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:30:08.69 +34:48:09.9: 12.02 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:30:08.69 +34:48:09.9: 12.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2046775495361598208,2461163.7894,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2046775495361598208 20260503.2894 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.41 20:00:20.71 +33:16:06.5
69.90147 1.70530 galactic Cyg Second-epoch detections are separated by 3.2" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0984+33.2667 | 20:00:23.62 +33:16:00.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:00:20.71 +33:16:06.5: 13.02 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:00:20.71 +33:16:06.5: 13.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0984+33.2667,2461163.7894,11.41,0.05,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 J300.0984+33.2667 20260503.2894 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 05 03.2894 2461163.7894 11.44 19:40:43.03 +33:21:18.7
67.89453 5.28427 galactic Cyg Second-epoch detections are separated by 4.8" and 4.0 pix
The object was found in VSX21" Gaia DR3 2046918333123670272
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.840 G 12.870 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:40:43.03 +33:21:18.7: 12.51 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:40:43.03 +33:21:18.7: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 2046918333123670272,2461163.7894,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2046918333123670272 20260503.2894 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.36 19:40:14.20 +31:03:20.4
65.83089 4.25031 galactic Cyg Second-epoch detections are separated by 3.5" 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 J295.0581+31.0439 | 19:40:11.91 +31:03:15.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1950ApJ...112...90M LF 2 +30 346
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:40:14.20 +31:03:20.4: 13.31 +/- 0.07 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:40:14.20 +31:03:20.4: 13.43 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 J295.0581+31.0439,2461163.7894,11.36,0.05,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
ATO J295.0581+31.0439 20260503.2894 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 05 03.2894 2461163.7894 11.50 19:25:11.19 +33:10:48.8
66.19504 8.06269 galactic Lyr Second-epoch detections are separated by 2.2" 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 J291.3089+33.1879 | 19:25:11.19 +33:11:20.6 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.053+/- (M)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:25:11.19 +33:10:48.8: 12.93 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:25:11.19 +33:10:48.8: 12.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J291.3089+33.1879,2461163.7894,11.50,0.05,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
ATO J291.3089+33.1879 20260503.2894 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 05 03.2894 2461163.7894 11.58 19:57:33.29 +30:53:08.2
67.56136 0.96083 galactic Cyg Second-epoch detections are separated by 4.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J195735.49+305330.7 | 19:57:35.51 +30:53:30.8 (Gaia DR3) | SR (local) | 231.362923000000 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:57:33.29 +30:53:08.2: 13.64 +/- 0.08 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:57:33.29 +30:53:08.2: 13.68 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.66 +/- 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
ASASSN-V J195735.49+305330.7,2461163.7894,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195735.49+305330.7 20260503.2894 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.56 19:44:57.50 +31:47:37.6
66.97244 3.73789 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 J296.2235+31.7887 | 19:44:55.40 +31:47:56.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:44:57.50 +31:47:37.6: 13.83 +/- 0.11 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:44:57.50 +31:47:37.6: 13.79 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 J296.2235+31.7887,2461163.7894,11.56,0.05,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 J296.2235+31.7887 20260503.2894 11.56CV 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 05 03.2894 2461163.7894 11.47 19:59:44.30 +33:03:06.7
69.65033 1.69952 galactic Cyg Second-epoch detections are separated by 3.0" and 4.5 pix
The object was found in VSX18" ZTF J195945.69+330306.7
Type: EB:
# Max. Min./Amp. JD0 Period
16.984 r Y 0.151 r 2458290.88370 21.301060400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:59:44.30 +33:03:06.7: 12.32 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:59:44.30 +33:03:06.7: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195945.69+330306.7,2461163.7894,11.47,0.05,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
ZTF J195945.69+330306.7 20260503.2894 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 05 03.2894 2461163.7894 11.48 19:41:15.87 +29:13:42.4
64.34475 3.15999 galactic Cyg Second-epoch detections are separated by 8.1" 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 | Gaia DR3 2031580283382973056 | 19:41:15.40 +29:14:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:41:15.87 +29:13:42.4: 12.38 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:41:15.87 +29:13:42.4: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2031580283382973056,2461163.7894,11.48,0.05,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
Gaia DR3 2031580283382973056 20260503.2894 11.48CV 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 05 03.2894 2461163.7894 11.55 19:35:45.00 +32:27:29.6
66.59951 5.76373 galactic Cyg Second-epoch detections are separated by 5.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2045317409836225024 | 19:35:43.21 +32:27:37.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:35:45.00 +32:27:29.6: 12.86 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:35:45.00 +32:27:29.6: 12.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2045317409836225024,2461163.7894,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2045317409836225024 20260503.2894 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.62 19:54:14.03 +31:50:02.8
68.00549 2.05862 galactic Cyg Second-epoch detections are separated by 5.5" 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 | Gaia DR3 2033833423212497152 | 19:54:12.49 +31:50:16.1 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:54:14.03 +31:50:02.8: 13.24 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:54:14.03 +31:50:02.8: 13.28 +/- 0.05 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
Gaia DR3 2033833423212497152,2461163.7894,11.62,0.05,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 2033833423212497152 20260503.2894 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 05 03.2894 2461163.7894 11.60 20:02:27.45 +34:49:56.1
71.46147 2.15918 galactic Cyg Second-epoch detections are separated by 7.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2058644830780050304 | 20:02:28.91 +34:50:19.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.496+/- (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:02:27.45 +34:49:56.1: 13.94 +/- 0.09 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:02:27.45 +34:49:56.1: 13.86 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.90 +/- 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
Large-amplitude variable Gaia DR2 2058644830780050304,2461163.7894,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2058644830780050304 20260503.2894 11.60CV 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 05 03.2894 2461163.7894 11.76 20:04:10.74 +31:07:40.0
68.51602 -0.11714 galactic Cyg Second-epoch detections are separated by 2.1" and 4.4 pix
The object was found in VSX19" ASASSN-V J200409.50+310729.5
Type: SR
# Max. Min./Amp. JD0 Period
12.050 V 12.750 V 2458252.67100 89.278354300000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:04:10.74 +31:07:40.0: 12.94 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:04:10.74 +31:07:40.0: 12.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J200409.50+310729.5,2461163.7894,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200409.50+310729.5 20260503.2894 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.78 19:45:21.63 +31:17:58.1
66.58560 3.41755 galactic Cyg Second-epoch detections are separated by 6.5" and 5.4 pix
The object was found in VSX17" Gaia DR3 2032996041994407808
Type: E
# Max. Min./Amp. JD0 Period
18.560 G 18.860 G 2.414420000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:45:21.63 +31:17:58.1: 13.75 +/- 0.09 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:45:21.63 +31:17:58.1: 13.85 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 2032996041994407808,2461163.7894,11.78,0.05,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 2032996041994407808 20260503.2894 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 05 03.2894 2461163.7894 11.80 19:47:01.69 +31:27:52.3
66.90699 3.19176 galactic Cyg Second-epoch detections are separated by 7.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.7629+31.4599 | 19:47:03.13 +31:27:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:47:01.69 +31:27:52.3: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:47:01.69 +31:27:52.3: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.7629+31.4599,2461163.7894,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.7629+31.4599 20260503.2894 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 05 03.2894 2461163.7894 11.71 19:40:32.05 +31:52:33.9
66.57984 4.59603 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 J295.1262+31.8833 | 19:40:30.24 +31:52:32.8 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:40:32.05 +31:52:33.9: 12.79 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:40:32.05 +31:52:33.9: 12.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.1262+31.8833,2461163.7894,11.71,0.05,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 J295.1262+31.8833 20260503.2894 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 05 03.2894 2461163.7894 11.78 19:54:25.63 +32:29:27.4
68.59011 2.36166 galactic Cyg Second-epoch detections are separated by 7.1" and 3.7 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 J298.6125+32.5089 | 19:54:26.91 +32:29:56.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:54:25.63 +32:29:27.4: 13.16 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:54:25.63 +32:29:27.4: 13.22 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.6125+32.5089,2461163.7894,11.78,0.05,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 J298.6125+32.5089 20260503.2894 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 05 03.2894 2461163.7894 11.76 19:39:19.71 +31:43:55.2
66.32830 4.74941 galactic Cyg Second-epoch detections are separated by 7.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.8191+31.7250 | 19:39:17.87 +31:43:50.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M8 1959ApJS....4...73W NSV 12273
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:39:19.71 +31:43:55.2: 13.09 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:39:19.71 +31:43:55.2: 13.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.8191+31.7250,2461163.7894,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.8191+31.7250 20260503.2894 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.86 19:47:38.21 +33:23:46.1
68.64642 4.04856 galactic Cyg Second-epoch detections are separated by 8.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.9105+33.4093 | 19:47:37.50 +33:24:12.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A 1925AnHar.100....1C HD 225814
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:47:38.21 +33:23:46.1: 12.96 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:47:38.21 +33:23:46.1: 13.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.9105+33.4093,2461163.7894,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.9105+33.4093 20260503.2894 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 05 03.2894 2461163.7894 11.81 20:18:27.52 +34:37:04.8
73.07805 -0.71168 galactic Cyg Second-epoch detections are separated by 1.0" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2055592036736530944 | 20:18:29.20 +34:37:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:18:27.52 +34:37:04.8: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:18:27.52 +34:37:04.8: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055592036736530944,2461163.7894,11.81,0.05,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
Gaia DR3 2055592036736530944 20260503.2894 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 05 03.2894 2461163.7894 11.83 19:43:13.55 +35:15:10.9
69.81240 5.75963 galactic Cyg Second-epoch detections are separated by 6.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2047749598264180352 | 19:43:13.90 +35:15:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.557+/- (K)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:43:13.55 +35:15:10.9: 13.32 +/- 0.07 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:43:13.55 +35:15:10.9: 12.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2047749598264180352,2461163.7894,11.83,0.05,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
Gaia DR3 2047749598264180352 20260503.2894 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 05 03.2894 2461163.7894 11.85 19:52:29.17 +33:57:52.8
69.64901 3.46541 galactic Cyg Second-epoch detections are separated by 5.6" 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 | Gaia DR3 2035197676620577792 | 19:52:28.78 +33:58:23.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:52:29.17 +33:57:52.8: 13.29 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:52:29.17 +33:57:52.8: 13.73 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2035197676620577792,2461163.7894,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2035197676620577792 20260503.2894 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.92 20:02:26.49 +31:38:59.2
68.76058 0.47461 galactic Cyg Second-epoch detections are separated by 2.9" and 4.7 pix
The object was found in VSX21" Gaia DR3 2030910955656023424
Type: L
# Max. Min./Amp. JD0 Period
17.660 G 17.800 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:02:26.49 +31:38:59.2: 13.42 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:02:26.49 +31:38:59.2: 13.34 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030910955656023424,2461163.7894,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030910955656023424 20260503.2894 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.81 19:34:57.89 +33:20:34.4
67.30197 6.33102 galactic Cyg Second-epoch detections are separated by 6.3" and 5.8 pix
The object was found in VSX21" Gaia DR3 2045698562403105280
Type: ROT
# Max. Min./Amp. JD0 Period
14.830 G 14.880 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:34:57.89 +33:20:34.4: 13.36 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:34:57.89 +33:20:34.4: 13.48 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 2045698562403105280,2461163.7894,11.81,0.05,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
Gaia DR3 2045698562403105280 20260503.2894 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 05 03.2894 2461163.7894 11.95 20:05:27.47 +32:02:22.4
69.43200 0.14073 galactic Cyg Second-epoch detections are separated by 5.4" 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 | ATO J301.3747+32.0581 | 20:05:29.89 +32:02:49.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:05:27.47 +32:02:22.4: 13.40 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:05:27.47 +32:02:22.4: 13.45 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.3747+32.0581,2461163.7894,11.95,0.05,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 J301.3747+32.0581 20260503.2894 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 05 03.2894 2461163.7894 11.82 19:35:33.30 +31:52:58.2
66.07214 5.52425 galactic Cyg Second-epoch detections are separated by 3.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.8986+31.8897 | 19:35:33.39 +31:53:21.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.505+/-0.145 (K)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:35:33.30 +31:52:58.2: 13.72 +/- 0.08 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:35:33.30 +31:52:58.2: 13.59 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 J293.8986+31.8897,2461163.7894,11.82,0.05,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 J293.8986+31.8897 20260503.2894 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 05 03.2894 2461163.7894 11.93 19:45:12.45 +29:19:15.7
64.85214 2.45921 galactic Cyg Second-epoch detections are separated by 5.1" and 4.7 pix
The object was found in VSX19" ZTF J194513.67+291926.2
Type: SR
# Max. Min./Amp. JD0 Period
14.662 r Y 0.056 r 2458326.97660 114.608070200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:45:12.45 +29:19:15.7: 13.01 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:45:12.45 +29:19:15.7: 13.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J194513.67+291926.2,2461163.7894,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194513.67+291926.2 20260503.2894 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 05 03.2894 2461163.7894 12.08 20:11:29.17 +31:19:33.1
69.52774 -1.32381 galactic Cyg Second-epoch detections are separated by 2.8" 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 | Gaia DR3 2054003757825294080 | 20:11:31.17 +31:19:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:11:29.17 +31:19:33.1: 14.08 +/- 0.09 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:11:29.17 +31:19:33.1: 14.21 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.14 +/- 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 2054003757825294080,2461163.7894,12.08,0.05,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
Gaia DR3 2054003757825294080 20260503.2894 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 05 03.2894 2461163.7894 12.26 20:10:46.93 +31:55:58.2
69.95374 -0.86615 galactic Cyg Second-epoch detections are separated by 8.0" and 3.1 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 J302.7001+31.9273 | 20:10:46.46 +31:56:17.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.227+/-0.040 (M)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:10:46.93 +31:55:58.2: 13.80 +/- 0.08 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:10:46.93 +31:55:58.2: 13.96 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.7001+31.9273,2461163.7894,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J302.7001+31.9273 20260503.2894 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 05 03.2894 2461163.7894 12.14 19:51:46.86 +32:59:02.6
68.72887 3.09213 galactic Cyg Second-epoch detections are separated by 3.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.9560+32.9994 | 19:51:48.66 +32:59:24.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:51:46.86 +32:59:02.6: 13.48 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:51:46.86 +32:59:02.6: 13.70 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 J297.9560+32.9994,2461163.7894,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.9560+32.9994 20260503.2894 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 05 03.2894 2461163.7894 12.28 19:41:58.17 +32:41:21.4
67.44027 4.72968 galactic Cyg Second-epoch detections are separated by 4.5" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2034871087306656128 | 19:41:56.16 +32:41:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.785+/-0.179 (K)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:41:58.17 +32:41:21.4: 14.01 +/- 0.12 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:41:58.17 +32:41:21.4: 13.98 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034871087306656128,2461163.7894,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034871087306656128 20260503.2894 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 05 03.2894 2461163.7894 12.20 19:47:53.16 +32:44:19.0
68.10245 3.67371 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 | Gaia DR3 2034732342686996992 | 19:47:53.20 +32:44:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.853+/-0.169 (M)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:47:53.16 +32:44:19.0: 14.32 +/- 0.16 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:47:53.16 +32:44:19.0: 14.20 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.25 +/- 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
Gaia DR3 2034732342686996992,2461163.7894,12.20,0.05,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
Gaia DR3 2034732342686996992 20260503.2894 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 05 03.2894 2461163.7894 12.32 19:27:05.70 +29:31:37.5
63.12153 6.01142 galactic Cyg Second-epoch detections are separated by 5.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2038589459494109696 | 19:27:03.93 +29:31:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:27:05.70 +29:31:37.5: 14.08 +/- 0.13 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:27:05.70 +29:31:37.5: 13.82 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2038589459494109696,2461163.7894,12.32,0.05,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
Gaia DR3 2038589459494109696 20260503.2894 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 05 03.2894 2461163.7894 12.34 19:59:44.12 +32:36:58.6
69.27913 1.47136 galactic Cyg Second-epoch detections are separated by 8.7" 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 | Gaia DR3 2034152792637120128 | 19:59:44.12 +32:37:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:59:44.12 +32:36:58.6: 13.82 +/- 0.09 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:59:44.12 +32:36:58.6: 13.79 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 2034152792637120128,2461163.7894,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034152792637120128 20260503.2894 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 05 03.2894 2461163.7894 11.99 19:52:31.81 +33:14:01.8
69.02416 3.08457 galactic Cyg Second-epoch detections are separated by 6.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J298.1180+33.2401 | 19:52:30.64 +33:13:47.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:52:31.81 +33:14:01.8: 13.98 +/- 0.11 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:52:31.81 +33:14:01.8: 13.75 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 J298.1180+33.2401,2461163.7894,11.99,0.05,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 J298.1180+33.2401 20260503.2894 11.99CV 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 05 03.2894 2461163.7894 11.34 19:46:04.14 +31:28:48.5
66.81802 3.37664 galactic Cyg Second-epoch detections are separated by 7.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.5200+31.4812 | 19:46:02.84 +31:28:37.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB 1954BOTT....2k..27I [IC54] 49
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:46:04.14 +31:28:48.5: 12.68 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:46:04.14 +31:28:48.5: 12.73 +/- 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 J296.5200+31.4812,2461163.7894,11.34,0.05,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
ATO J296.5200+31.4812 20260503.2894 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 05 03.2894 2461163.7894 11.58 19:52:57.82 +28:27:30.9
64.96827 0.55857 galactic Vul Second-epoch detections are separated by 5.2" and 5.2 pix
The object was found in VSX22" Gaia DR3 2028443685935322368
Type: ROT
# Max. Min./Amp. JD0 Period
15.670 G 15.710 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:52:57.82 +28:27:30.9: 13.04 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:52:57.82 +28:27:30.9: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2028443685935322368,2461163.7894,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028443685935322368 20260503.2894 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.13 19:50:16.04 +33:51:20.8
69.32077 3.80669 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 | ZTF J195016.38+335211.2 | 19:50:15.01 +33:52:04.2 (Gaia DR3) | EW (local) | 2458330.87470 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:50:16.04 +33:51:20.8: 12.42 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:50:16.04 +33:51:20.8: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.27 +/- 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
ZTF J195016.38+335211.2,2461163.7894,11.13,0.05,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
ZTF J195016.38+335211.2 20260503.2894 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 05 03.2894 2461163.7894 11.55 19:45:32.60 +28:21:27.1
64.05384 1.91387 galactic Vul Second-epoch detections are separated by 1.5" and 4.8 pix
The object was found in VSX11" ZTF J194533.10+282118.1
Type: EW
# Max. Min./Amp. JD0 Period
19.352 r Y 0.824 r 2458650.83890 0.315732000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:45:32.60 +28:21:27.1: 12.83 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:45:32.60 +28:21:27.1: 12.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194533.10+282118.1,2461163.7894,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194533.10+282118.1 20260503.2894 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.74 19:41:03.44 +30:36:50.4
65.53143 3.88034 galactic Cyg Second-epoch detections are separated by 5.9" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2032846847702801920 | 19:41:01.66 +30:37:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1950ApJ...112...90M LF 2 +30 375
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:41:03.44 +30:36:50.4: 13.08 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:41:03.44 +30:36:50.4: 13.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.14 +/- 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
Gaia DR3 2032846847702801920,2461163.7894,11.74,0.05,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 2032846847702801920 20260503.2894 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 05 03.2894 2461163.7894 11.67 19:54:42.55 +33:10:20.8
69.20543 2.66177 galactic Cyg Second-epoch detections are separated by 2.8" and 4.1 pix
The object was found in VSX16" Gaia DR3 2034346482824280064
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.320 G 12.350 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:54:42.55 +33:10:20.8: 12.77 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:54:42.55 +33:10:20.8: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2034346482824280064,2461163.7894,11.67,0.05,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
Gaia DR3 2034346482824280064 20260503.2894 11.67CV 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 05 03.2894 2461163.7894 11.94 19:45:22.21 +31:18:19.0
66.59167 3.41865 galactic Cyg Second-epoch detections are separated by 2.7" 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 J296.3539+31.3067 | 19:45:23.28 +31:18:35.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:45:22.21 +31:18:19.0: 13.33 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:45:22.21 +31:18:19.0: 13.40 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.3539+31.3067,2461163.7894,11.94,0.05,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 J296.3539+31.3067 20260503.2894 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 05 03.2894 2461163.7894 11.48 19:34:29.26 +33:42:34.3
67.57900 6.59282 galactic Cyg Second-epoch detections are separated by 8.6" 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 J293.6187+33.7041 | 19:34:28.82 +33:42:58.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:34:29.26 +33:42:34.3: 12.47 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:34:29.26 +33:42:34.3: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.6187+33.7041,2461163.7894,11.48,0.05,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 J293.6187+33.7041 20260503.2894 11.48CV 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 05 03.2894 2461163.7894 11.87 19:28:27.26 +33:20:37.0
66.65900 7.53160 galactic Cyg Second-epoch detections are separated by 3.0" 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 | Large-amplitude variable Gaia DR2 2046398848223743232 | 19:28:27.72 +33:21:08.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:28:27.26 +33:20:37.0: 13.47 +/- 0.08 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:28:27.26 +33:20:37.0: 13.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2046398848223743232,2461163.7894,11.87,0.05,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
Large-amplitude variable Gaia DR2 2046398848223743232 20260503.2894 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 05 03.2894 2461163.7894 11.42 19:42:15.86 +31:17:50.3
66.25537 3.99101 galactic Cyg Second-epoch detections are separated by 4.5" 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 | V0463 Cyg | 19:42:13.92 +31:18:02.5 (Gaia DR3) | EA/DM (local) | 2.117562000000 (local) | Gaia3var=NOT_AVAILABLE SpType: A0 1950ApJ...112...90M LF 2 +31 272
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:42:15.86 +31:17:50.3: 12.53 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:42:15.86 +31:17:50.3: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0463 Cyg,2461163.7894,11.42,0.05,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
V0463 Cyg 20260503.2894 11.42CV 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 05 03.2894 2461163.7894 11.51 19:27:25.76 +35:14:11.6
68.25728 8.59174 galactic Cyg Second-epoch detections are separated by 2.7" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.8482+35.2429 | 19:27:25.88 +35:14:42.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.711+/-0.032 (K)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:27:25.76 +35:14:11.6: 12.91 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:27:25.76 +35:14:11.6: 12.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J291.8482+35.2429,2461163.7894,11.51,0.05,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
ATO J291.8482+35.2429 20260503.2894 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 05 03.2894 2461163.7894 11.73 19:50:23.78 +33:15:04.3
68.81188 3.47756 galactic Cyg Second-epoch detections are separated by 2.0" and 4.4 pix
The object was found in VSX21" Gaia DR3 2034764469044895744
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.180 G 12.210 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:50:23.78 +33:15:04.3: 12.92 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:50:23.78 +33:15:04.3: 12.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2034764469044895744,2461163.7894,11.73,0.05,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 2034764469044895744 20260503.2894 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 05 03.2894 2461163.7894 11.71 19:56:15.87 +34:35:55.0
70.59536 3.12128 galactic Cyg Second-epoch detections are separated by 2.5" and 4.2 pix
The object was found in VSX 4" ZTF J195615.58+343557.2
Type: EW
# Max. Min./Amp. JD0 Period
19.009 g Y 0.711 g 2458586.96430 0.502099200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:56:15.87 +34:35:55.0: 12.94 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:56:15.87 +34:35:55.0: 12.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 J195615.58+343557.2,2461163.7894,11.71,0.05,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
ZTF J195615.58+343557.2 20260503.2894 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 05 03.2894 2461163.7894 11.60 19:40:14.66 +33:04:03.6
67.59398 5.23060 galactic Cyg Second-epoch detections are separated by 5.7" 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 J295.0542+33.0811 | 19:40:13.46 +33:04:26.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:40:14.66 +33:04:03.6: 12.83 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:40:14.66 +33:04:03.6: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.0542+33.0811,2461163.7894,11.60,0.05,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 J295.0542+33.0811 20260503.2894 11.60CV 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 05 03.2894 2461163.7894 11.79 19:43:35.56 +31:45:05.4
66.79139 3.96898 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 J295.9004+31.7618 | 19:43:33.58 +31:45:23.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:43:35.56 +31:45:05.4: 13.94 +/- 0.12 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:43:35.56 +31:45:05.4: 14.01 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 J295.9004+31.7618,2461163.7894,11.79,0.05,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 J295.9004+31.7618 20260503.2894 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 05 03.2894 2461163.7894 11.62 19:40:13.26 +32:55:20.3
67.46409 5.16411 galactic Cyg Second-epoch detections are separated by 2.4" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2045401793025193856 | 19:40:11.35 +32:55:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:40:13.26 +32:55:20.3: 12.54 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:40:13.26 +32:55:20.3: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2045401793025193856,2461163.7894,11.62,0.05,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 2045401793025193856 20260503.2894 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 05 03.2894 2461163.7894 12.46 19:25:12.32 +27:08:48.2
60.81160 5.26657 galactic Vul Second-epoch detections are separated by 5.2" 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 2025722802630044288 | 19:25:10.97 +27:09:15.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:25:12.32 +27:08:48.2: 13.72 +/- 0.09 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:25:12.32 +27:08:48.2: 13.71 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 2025722802630044288,2461163.7894,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2025722802630044288 20260503.2894 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 05 03.2894 2461163.7894 11.48 19:55:34.35 +32:58:44.2
69.13289 2.40701 galactic Cyg Second-epoch detections are separated by 5.0" and 3.7 pix
The object was found in VSX17" V1459 Cyg
Type: I:
# Max. Min./Amp. JD0 Period
14.400 pg 15.700 pg 730.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:55:34.35 +32:58:44.2: 12.46 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:55:34.35 +32:58:44.2: 12.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1459 Cyg,2461163.7894,11.48,0.05,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
V1459 Cyg 20260503.2894 11.48CV 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 05 03.2894 2461163.7894 11.87 19:41:26.61 +29:34:26.9
64.66533 3.29630 galactic Cyg Second-epoch detections are separated by 1.9" and 4.4 pix
The object was found in VSX18" Gaia DR3 2031658554852185216
Type:
# Max. Min./Amp. JD0 Period
20.160 G 20.700 G 0.253223000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:41:26.61 +29:34:26.9: 13.46 +/- 0.08 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:41:26.61 +29:34:26.9: 13.41 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.44 +/- 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 2031658554852185216,2461163.7894,11.87,0.05,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
Gaia DR3 2031658554852185216 20260503.2894 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 05 03.2894 2461163.7894 11.77 19:35:22.32 +33:24:16.2
67.39722 6.28565 galactic Cyg Second-epoch detections are separated by 7.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.8445+33.3970 | 19:35:20.78 +33:24:22.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:35:22.32 +33:24:16.2: 12.72 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:35:22.32 +33:24:16.2: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.8445+33.3970,2461163.7894,11.77,0.05,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 J293.8445+33.3970 20260503.2894 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 05 03.2894 2461163.7894 12.48 19:35:38.77 +31:57:26.1
66.14707 5.54295 galactic Cyg Second-epoch detections are separated by 6.3" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.8900+31.9675 | 19:35:35.63 +31:57:33.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:35:38.77 +31:57:26.1: 13.76 +/- 0.10 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:35:38.77 +31:57:26.1: 13.78 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 J293.8900+31.9675,2461163.7894,12.48,0.05,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 J293.8900+31.9675 20260503.2894 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 05 03.2894 2461163.7894 11.69 19:48:38.96 +31:02:37.7
66.71736 2.68069 galactic Cyg Second-epoch detections are separated by 4.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.1471+31.0351 | 19:48:37.33 +31:02:40.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:48:38.96 +31:02:37.7: 12.82 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:48:38.96 +31:02:37.7: 12.73 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 J297.1471+31.0351,2461163.7894,11.69,0.05,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
ATO J297.1471+31.0351 20260503.2894 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 05 03.2894 2461163.7894 11.27 19:39:43.04 +32:53:33.7
67.38648 5.24206 galactic Cyg Second-epoch detections are separated by 2.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.9090+32.8975 | 19:39:41.21 +32:53:54.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:39:43.04 +32:53:33.7: 12.45 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:39:43.04 +32:53:33.7: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.9090+32.8975,2461163.7894,11.27,0.05,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
ATO J294.9090+32.8975 20260503.2894 11.27CV 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 05 03.2894 2461163.7894 12.03 19:26:31.77 +32:34:13.2
65.77907 7.53200 galactic Cyg Second-epoch detections are separated by 5.9" 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 J291.6344+32.5832 | 19:26:30.56 +32:34:24.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:26:31.77 +32:34:13.2: 13.06 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:26:31.77 +32:34:13.2: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J291.6344+32.5832,2461163.7894,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J291.6344+32.5832 20260503.2894 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 05 03.2894 2461163.7894 11.53 19:24:35.82 +34:45:15.5
67.55558 8.88843 galactic Lyr Second-epoch detections are separated by 5.5" 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 | ATO J291.1501+34.7601 | 19:24:36.03 +34:45:36.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:24:35.82 +34:45:15.5: 12.89 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:24:35.82 +34:45:15.5: 12.47 +/- 0.03 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 J291.1501+34.7601,2461163.7894,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J291.1501+34.7601 20260503.2894 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.81 19:37:07.99 +30:40:26.5
65.17154 4.64663 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 | ZTF J193705.15+304035.1 | 19:37:06.31 +30:40:24.7 (Gaia DR3) | EW (local) | 2458275.94310 (local) | Gaia3var=NOT_AVAILABLE SpType: A2 1950ApJ...112...90M LF 2 +30 242
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:37:07.99 +30:40:26.5: 12.93 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:37:07.99 +30:40:26.5: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J193705.15+304035.1,2461163.7894,11.81,0.05,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
ZTF J193705.15+304035.1 20260503.2894 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 05 03.2894 2461163.7894 11.80 19:40:36.41 +34:20:43.2
68.75239 5.78610 galactic Cyg Second-epoch detections are separated by 2.9" 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 J295.1309+34.3429 | 19:40:34.40 +34:20:42.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:40:36.41 +34:20:43.2: 12.85 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:40:36.41 +34:20:43.2: 12.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.1309+34.3429,2461163.7894,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.1309+34.3429 20260503.2894 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 05 03.2894 2461163.7894 12.09 19:48:27.49 +28:26:19.9
64.44670 1.40073 galactic Vul Second-epoch detections are separated by 5.5" and 3.6 pix
The object was found in VSX 9" Gaia DR3 2028663931836419200
Type: L
# Max. Min./Amp. JD0 Period
17.770 G 18.180 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:48:27.49 +28:26:19.9: 12.92 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:48:27.49 +28:26:19.9: 13.08 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2028663931836419200,2461163.7894,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028663931836419200 20260503.2894 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 05 03.2894 2461163.7894 11.62 19:47:16.68 +31:43:23.7
67.15791 3.27546 galactic Cyg Second-epoch detections are separated by 5.3" and 5.5 pix
The object was found in VSX24" Gaia DR3 2034515223495363968
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.220 G 11.240 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:47:16.68 +31:43:23.7: 12.58 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:47:16.68 +31:43:23.7: 12.62 +/- 0.03 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
Gaia DR3 2034515223495363968,2461163.7894,11.62,0.05,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 2034515223495363968 20260503.2894 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 05 03.2894 2461163.7894 11.86 20:07:31.71 +29:35:47.0
67.61203 -1.54897 galactic Cyg Second-epoch detections are separated by 4.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2029727327054824576 | 20:07:31.96 +29:36:09.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:07:31.71 +29:35:47.0: 13.83 +/- 0.08 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:07:31.71 +29:35:47.0: 13.84 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 2029727327054824576,2461163.7894,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2029727327054824576 20260503.2894 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 05 03.2894 2461163.7894 11.42 19:45:44.10 +35:16:36.0
70.08649 5.32551 galactic Cyg Second-epoch detections are separated by 7.4" and 4.0 pix
The object was found in VSX 5" Gaia DR3 2047576901905689984
Type: E
# Max. Min./Amp. JD0 Period
17.830 G 18.240 G 0.412298000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:45:44.10 +35:16:36.0: 13.38 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:45:44.10 +35:16:36.0: 12.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2047576901905689984,2461163.7894,11.42,0.05,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
Gaia DR3 2047576901905689984 20260503.2894 11.42CV 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 05 03.2894 2461163.7894 12.04 19:30:46.58 +29:49:14.3
63.75985 5.44380 galactic Cyg Second-epoch detections are separated by 8.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2032607016727356032 | 19:30:44.70 +29:49:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9 1950ApJ...112...90M LF 2 +29 45
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:30:46.58 +29:49:14.3: 13.31 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:30:46.58 +29:49:14.3: 13.48 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 2032607016727356032,2461163.7894,12.04,0.05,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 2032607016727356032 20260503.2894 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 05 03.2894 2461163.7894 11.72 19:47:46.48 +32:38:46.7
68.01067 3.64764 galactic Cyg Second-epoch detections are separated by 1.1" and 4.8 pix
The object was found in VSX18" ZTF J194747.65+323835.9
Type: EW
# Max. Min./Amp. JD0 Period
19.264 r Y 0.369 r 2458217.98780 0.345253800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:47:46.48 +32:38:46.7: 13.35 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:47:46.48 +32:38:46.7: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194747.65+323835.9,2461163.7894,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194747.65+323835.9 20260503.2894 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.83 19:37:48.66 +34:09:58.0
68.31393 6.20530 galactic Cyg Second-epoch detections are separated by 1.8" 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 J294.4380+34.1730 | 19:37:48.10 +34:10:19.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:37:48.66 +34:09:58.0: 12.84 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:37:48.66 +34:09:58.0: 12.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.4380+34.1730,2461163.7894,11.83,0.05,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 J294.4380+34.1730 20260503.2894 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 05 03.2894 2461163.7894 11.54 19:30:57.43 +34:39:45.2
68.08041 7.68543 galactic Cyg Second-epoch detections are separated by 3.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2046761274739081984 | 19:30:55.79 +34:39:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:30:57.43 +34:39:45.2: 12.82 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:30:57.43 +34:39:45.2: 12.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.75 +/- 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 2046761274739081984,2461163.7894,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2046761274739081984 20260503.2894 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 12.40 19:25:51.34 +29:54:15.6
63.33118 6.42529 galactic Cyg Second-epoch detections are separated by 6.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.4679+29.9013 | 19:25:49.96 +29:54:34.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:25:51.34 +29:54:15.6: 13.93 +/- 0.11 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:25:51.34 +29:54:15.6: 13.70 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 J291.4679+29.9013,2461163.7894,12.40,0.05,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 J291.4679+29.9013 20260503.2894 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 05 03.2894 2461163.7894 11.19 20:06:31.36 +34:31:36.7
71.64955 1.28948 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 | Gaia DR3 2058399674046327808 | 20:06:32.55 +34:31:59.3 (Gaia DR3) | BE/GCAS/S (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:06:31.36 +34:31:36.7: 12.35 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:06:31.36 +34:31:36.7: 12.05 +/- 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
Gaia DR3 2058399674046327808,2461163.7894,11.19,0.05,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
Gaia DR3 2058399674046327808 20260503.2894 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 05 03.2894 2461163.7894 11.79 19:31:11.28 +33:11:46.0
66.79609 6.95736 galactic Cyg Second-epoch detections are separated by 5.1" 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 J292.7977+33.2138 | 19:31:11.63 +33:12:19.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:31:11.28 +33:11:46.0: 12.98 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:31:11.28 +33:11:46.0: 12.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.7977+33.2138,2461163.7894,11.79,0.05,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 J292.7977+33.2138 20260503.2894 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 05 03.2894 2461163.7894 11.84 19:54:10.85 +33:02:04.2
69.03002 2.68568 galactic Cyg Second-epoch detections are separated by 6.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2034320747389086080 | 19:54:09.79 +33:02:32.4 (Gaia DR3) | (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:54:10.85 +33:02:04.2: 12.94 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:54:10.85 +33:02:04.2: 13.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2034320747389086080,2461163.7894,11.84,0.05,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 2034320747389086080 20260503.2894 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 05 03.2894 2461163.7894 12.12 20:01:12.06 +32:21:14.6
69.21895 1.07052 galactic Cyg Second-epoch detections are separated by 2.6" and 4.5 pix
The object was found in VSX15" ASASSN-V J200110.84+322116.4
Type: SR
# Max. Min./Amp. JD0 Period
12.690 V 12.920 V 2458252.62220 76.733935700000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:01:12.06 +32:21:14.6: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:01:12.06 +32:21:14.6: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J200110.84+322116.4,2461163.7894,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200110.84+322116.4 20260503.2894 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 05 03.2894 2461163.7894 11.24 19:42:53.61 +33:51:17.6
68.55475 5.13349 galactic Cyg Second-epoch detections are separated by 2.1" 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 2047049999641377408 | 19:42:52.64 +33:51:41.8 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A 1925AnHar.100....1C HD 225478
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:42:53.61 +33:51:17.6: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:42:53.61 +33:51:17.6: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.27 +/- 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
Gaia DR3 2047049999641377408,2461163.7894,11.24,0.05,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 2047049999641377408 20260503.2894 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 05 03.2894 2461163.7894 11.97 19:46:23.26 +32:12:45.3
67.48762 3.68386 galactic Cyg Second-epoch detections are separated by 1.9" 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 | Gaia DR3 2034611430769330560 | 19:46:21.82 +32:13:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:46:23.26 +32:12:45.3: 13.37 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:46:23.26 +32:12:45.3: 13.45 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034611430769330560,2461163.7894,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034611430769330560 20260503.2894 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 11.33 19:31:55.43 +34:00:57.9
67.59823 7.20673 galactic Cyg Second-epoch detections are separated by 4.4" and 5.4 pix
The object was found in VSX22" Gaia DR3 2046536935698424320
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
18.120 G 18.360 G 0.085874700000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:31:55.43 +34:00:57.9: 12.68 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:31:55.43 +34:00:57.9: 12.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.57 +/- 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 2046536935698424320,2461163.7894,11.33,0.05,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
Gaia DR3 2046536935698424320 20260503.2894 11.33CV 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 05 03.2894 2461163.7894 11.44 19:49:22.87 +31:50:17.6
67.48278 2.94719 galactic Cyg Second-epoch detections are separated by 2.0" and 4.4 pix
The object was found in VSX19" Gaia DR3 2033793050521342720
Type: E
# Max. Min./Amp. JD0 Period
18.980 G 19.290 G 0.511360000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:49:22.87 +31:50:17.6: 12.37 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:49:22.87 +31:50:17.6: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2033793050521342720,2461163.7894,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2033793050521342720 20260503.2894 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2894 2461163.7894 12.21 19:31:59.16 +27:32:26.7
61.87408 4.12584 galactic Vul 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 J292.9836+27.5466 | 19:31:57.82 +27:33:02.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:31:59.16 +27:32:26.7: 13.20 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:31:59.16 +27:32:26.7: 13.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.9836+27.5466,2461163.7894,12.21,0.05,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
ATO J292.9836+27.5466 20260503.2894 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461140.86966602 10.04.2026 08:52:09.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
First image: 2461140.86966602 10.04.2026 08:52:09.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
Last image: 2461163.78970669 03.05.2026 06:57:00.658 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.09
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: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 25034
Objects passed selection criteria: 24921
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 17298.5
Average stars matched: 16833.8 (97.3134 %)
Memory usage VmPeak: 129072 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 01:59:26 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: 2461140.86966602 10.04.2026 08:52:09.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
First image: 2461140.86966602 10.04.2026 08:52:09.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
Last image: 2461163.78970669 03.05.2026 06:57:00.658 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 463
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
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: 42 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 214159
Objects passed selection criteria: 213420
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 144835
Average stars matched: 138102 (95.3513 %)
Memory usage VmPeak: 2233104 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 02:06:32 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
SExtractor catalog cache: saved Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.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-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.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: 2461163.78902543
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-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits exists and is non-empty
Saving wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits to local_wcs_cache/
'wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits'
wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits exists and is non-empty
Saving wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits to local_wcs_cache/
'wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits'
wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits'
wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits (1st reference image)
verification OK: wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
Image size: 941.9'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 20:00:00.314 +30:00:03.04 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits (1st new image)
verification OK: wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
Image size: 942.8'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 20:00:22.870 +30:01:53.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:00:00.314 +30:00:03.04
Second-epoch image center 20:00:22.870 +30:01:53.16
Angular distance between the image centers 0.0869 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits (2nd new image)
verification OK: wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
Image size: 942.8'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 20:00:24.020 +30:01:30.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:00:00.314 +30:00:03.04
Second-epoch image center 20:00:24.020 +30:01:30.77
Angular distance between the image centers 0.0889 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 20:00:22.870 +30:01:53.16
Second-epoch second image center 20:00:24.020 +30:01:30.77
Angular distance between the image centers 0.00748 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits &> /tmp/tmp.tkn2q0vURA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits &> /tmp/tmp.stfXpnfCPM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits &> /tmp/tmp.OsZ1FthaB0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits &> /tmp/tmp.8ErFhYAOs0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.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-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits and wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat
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-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits and wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat
Found non-empty wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits and wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat
The reference image (wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits) and catalog (wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat) found
'wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat' -> 'wcsmag.cat'
Read 27028 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 290.8397 to 309.8729 deg, Dec +24.0038 to +35.4803 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 290.8397 to 309.8729 deg, Dec 24.0038 to 35.4803 deg
Loaded 31152 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): 14675 out of 16028 total matches.
Matched with Tycho-2 16028 out of 27028 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.743800
a=0.000000 b=1.000000 c=22.743800
From vast_summary.log: estimated ref. image limiting mag.: -8.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.65
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.65
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27028 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 290.8397 to 309.8729 deg, Dec +24.0038 to +35.4803 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 290.8397 to 309.8729 deg, Dec 24.0038 to 35.4803 deg
Loaded 31152 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): 14675 out of 16028 total matches.
Matched with Tycho-2 16028 out of 27028 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits:
Forced-photometry filter: calibrated wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits -> calib.txt_param_ref_wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits (aperture=6.4)
Read 26881 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 290.8532 to 309.8966 deg, Dec +23.9794 to +35.4830 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 290.8532 to 309.8966 deg, Dec 23.9794 to 35.4830 deg
Loaded 31225 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): 17614 out of 19349 total matches.
Matched with Tycho-2 19349 out of 26881 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits:
Forced-photometry filter: calibrated wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits -> calib.txt_param_ref_wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
2.4 pix Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
5.5 pix fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
5.5 pix fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
2.4 pix wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
2.4 pix wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
Limiting magnitude estimates:
14.7 mag. Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
14.7 mag. Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
13.0 mag. fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
13.0 mag. fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 10.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.tkn2q0vURA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.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-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits' -> 'wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
WCS-calibrated image found: wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
Checking if the catalog wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat corresponding to the image wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat corresponding to the image wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits
WCS catalog name: wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3198, passed=27028
Got 27028 stars (including 23796 good ones) from the SExtractor catalog wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat
util/solve_plate_with_UCAC5 got 27028 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 25647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 25647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 25645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 940 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits -region wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.stfXpnfCPM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.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-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits' -> 'wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
WCS-calibrated image found: wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
Checking if the catalog wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits.cat corresponding to the image wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits.cat corresponding to the image wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits
WCS catalog name: wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3209, passed=26881
Got 26881 stars (including 23647 good ones) from the SExtractor catalog wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits.cat
util/solve_plate_with_UCAC5 got 26881 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 25568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 25569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 25569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 935 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits -region wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OsZ1FthaB0 (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_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.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_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
Checking if the catalog wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits.cat corresponding to the image wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits.cat corresponding to the image wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
WCS catalog name: wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=851, passed=8003
Got 8003 stars (including 7152 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits.cat
util/solve_plate_with_UCAC5 got 8003 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.8'
Seting catalog search parameters based on the expected field of view 942.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013094 (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 0.010476 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 7698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 7696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 7713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.00"
Excluding outliers - 927 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits -region wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8ErFhYAOs0 (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_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.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_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
Checking if the catalog wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits.cat corresponding to the image wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits.cat corresponding to the image wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
WCS catalog name: wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=855, passed=8022
Got 8022 stars (including 7166 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits.cat
util/solve_plate_with_UCAC5 got 8022 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.8'
Seting catalog search parameters based on the expected field of view 942.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013094 (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 0.010476 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 7710 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 7712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 7719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 925 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits -region wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-56-01_20.00sec_-4.90C_LIGHTs_0164.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-08-Q1b1x1_015755_TTUQ1b1x1_1839775_Q6kXaM76/wcs_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165.fits'
Preparing the HTML report for the field Cyg-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:36:18.20 +29:55:41.8: 10.30 +/- 0.01 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 20:17:15.23 +34:20:01.4: 10.04 +/- 0.00 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:25:19.40 +31:53:13.6: 10.04 +/- 0.00 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:40:03.67 +34:40:51.0: 11.31 +/- 0.01 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-52-09_20.00sec_-4.90C_LIGHTs_0218.fits at 19:54:57.80 +34:55:37.3: 9.39 +/- 0.00 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:36:18.20 +29:55:41.8: 10.31 +/- 0.00 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 20:17:15.23 +34:20:01.4: 9.86 +/- 0.00 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:25:19.40 +31:53:13.6: 10.05 +/- 0.00 detection
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:40:03.67 +34:40:51.0: 11.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.31 +/- 0.00
Forced photometry reference-image weighted average: 9.93 +/- 0.00
Forced photometry filter REJECTED candidate at 19:36:18.20 +29:55:41.8: ref_mag=10.31 +/- 0.00 new_mean_mag=10.4270 delta=-0.12 (need > 0.90)
Forced photometry reference-image weighted average: 10.05 +/- 0.00
Forced photometry filter REJECTED candidate at 20:17:15.23 +34:20:01.4: ref_mag=9.93 +/- 0.00 new_mean_mag=10.0861 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 11.26 +/- 0.01
Forced photometry filter REJECTED candidate at 19:25:19.40 +31:53:13.6: ref_mag=10.05 +/- 0.00 new_mean_mag=10.1624 delta=-0.11 (need > 0.90)
Forced photometry filter KEPT candidate at 19:40:03.67 +34:40:51.0: ref_mag=11.26 +/- 0.01 new_mean_mag=10.2155 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cyg-08-Q1b1x1_2026-04-10_03-53-19_20.00sec_-4.90C_LIGHTs_0219.fits at 19:54:57.80 +34:55:37.3: 10.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.55 +/- 0.00
Forced photometry filter REJECTED candidate at 19:54:57.80 +34:55:37.3: ref_mag=9.55 +/- 0.00 new_mean_mag=9.7751 delta=-0.23 (need > 0.90)
Adding exclusion_list_local.txt__out30219.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31765_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 31765_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:32:03.90 +28:05:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31767_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 31767_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31769_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 31769_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31771_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 31771_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30219_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 30219_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23858_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 23858_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271791_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271791_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271792_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271792_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271802_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271802_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271807_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271807_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271809_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271809_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271811_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271811_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271817_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271817_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271820_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271820_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271825_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271825_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:32:16.09 +26:59:04.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271833_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271833_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271835_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271835_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271837_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271837_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271838_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271838_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271842_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271842_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271844_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 271844_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271851_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271851_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271854_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271854_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271858_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271858_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271861_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 271861_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271863_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271863_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271865_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271865_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271866_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271866_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271868_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271868_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271872_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271872_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271873_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271873_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271874_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271874_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271877_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271877_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271879_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271879_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271880_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271880_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271881_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271881_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271886_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271886_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271888_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271888_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271889_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271889_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271894_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271894_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:27:33.99 +25:01:20.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271899_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271899_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271900_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271900_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271901_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271901_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271903_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271903_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271907_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271907_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271909_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271909_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271917_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271917_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271922_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 271922_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271932_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271932_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271937_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271937_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271938_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271938_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271942_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271942_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271949_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271949_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271950_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 271950_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271956_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271956_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271958_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 271958_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271959_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271959_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271963_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271963_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271965_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271965_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271968_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271968_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271969_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271969_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271970_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271970_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271971_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271971_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271974_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271974_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271983_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271983_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271984_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271984_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 19:45:04.67 +27:30:51.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271985_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271985_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271987_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271987_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271990_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271990_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271992_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271992_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271993_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271993_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271994_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271994_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271999_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 271999_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272002_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272002_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272003_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272003_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272006_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272006_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272007_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272007_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272012_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272012_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272015_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272015_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272017_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272017_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272020_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272020_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272021_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272021_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272023_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272023_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272029_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272029_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272036_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272036_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272037_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272037_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272043_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272043_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272044_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272044_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272047_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272047_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272049_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272049_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272056_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272056_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272058_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272058_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272061_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272061_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272063_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272063_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272070_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272070_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272071_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272071_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272072_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272072_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272074_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272074_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272080_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272080_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272087_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272087_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272088_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272088_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272089_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272089_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272091_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272091_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272092_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272092_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272095_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272095_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272101_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272101_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272104_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272104_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272105_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272105_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272107_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272107_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272109_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272109_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272110_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272110_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272112_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272112_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272113_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272113_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272116_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272116_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272117_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272117_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272118_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272118_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272119_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272119_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272120_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272120_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272121_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272121_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272124_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272124_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272125_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272125_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272126_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272126_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272135_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272135_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272140_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272140_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272142_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272142_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272144_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272144_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272152_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272152_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272153_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272153_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272155_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272155_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272156_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272156_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272157_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272157_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272158_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272158_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272159_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272159_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272160_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272160_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272162_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272162_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272163_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272163_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272167_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272167_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272177_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272177_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272179_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272179_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272180_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272180_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272183_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272183_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272184_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272184_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272185_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272185_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272191_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272191_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272192_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272192_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272194_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272194_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272197_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272197_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272202_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272202_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272203_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272203_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272204_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272204_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272208_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272208_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272210_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272210_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272211_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272211_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272212_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272212_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272216_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272216_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272220_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272220_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272225_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272225_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272227_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272227_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272228_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272228_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272232_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272232_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272238_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272238_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 19:25:23.56 +28:38:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272239_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272239_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272248_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272248_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272249_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272249_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272254_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272254_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272261_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272261_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272263_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272263_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272264_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272264_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272265_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272265_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272285_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272285_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272288_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272288_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 19:28:26.92 +28:28:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272290_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272290_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272299_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272299_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272301_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272301_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272305_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272305_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272306_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272306_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272307_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272307_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272308_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272308_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272309_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272309_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272314_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272314_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272315_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272315_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272317_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272317_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272318_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272318_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272325_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272325_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272330_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272330_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272332_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272332_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272333_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272333_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272338_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272338_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272342_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272342_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272343_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272343_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272347_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272347_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:15:58.99 +34:02:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272406_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272406_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:32:03.99 +28:05:02.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272434_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272434_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272451_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272451_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272455_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272455_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272461_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272461_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272471_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272471_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272482_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272482_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272484_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272484_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272489_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272489_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272490_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272490_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272493_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272493_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272514_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272514_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272523_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272523_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272525_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272525_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272536_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272536_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272545_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272545_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272565_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272565_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272568_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272568_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272570_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272570_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272577_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272577_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272579_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272579_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272580_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272580_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272581_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272581_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272582_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272582_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272593_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272593_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272595_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272595_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272602_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272602_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272609_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272609_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272614_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272614_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272615_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272615_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272619_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272619_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272623_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272623_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272626_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272626_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272633_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272633_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272643_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272643_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272644_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272644_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272652_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272652_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272659_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272659_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272661_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272661_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272663_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272663_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272672_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272672_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272690_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272690_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272692_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272692_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272701_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272701_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272703_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272703_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272712_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272712_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272716_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272716_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272721_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272721_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272729_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272729_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272730_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272730_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272733_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272733_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272739_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272739_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272740_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272740_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272759_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272759_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272768_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272768_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272774_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272774_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272781_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272781_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272801_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272801_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272802_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272802_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272803_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272803_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:31:24.29 +24:49:28.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272857_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272857_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272863_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272863_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272864_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272864_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272876_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272876_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272892_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272892_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272896_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272896_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272899_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272899_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272902_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272902_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272905_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272905_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272906_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 272906_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272943_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 272943_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68054_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 68054_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:33:36.35 +27:17:54.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73166_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 73166_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193774_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 193774_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120608_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 120608_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172717_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 172717_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90067_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 90067_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249284_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 249284_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249491_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 249491_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249690_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 249690_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249901_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 249901_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110525_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 110525_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 230385_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 230385_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70508_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 70508_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191809_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 191809_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225383_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 225383_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218909_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 218909_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:36:28.54 +33:26:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175457_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 175457_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128302_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 128302_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46713_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 46713_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29499_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 29499_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137629_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 137629_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160508_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 160508_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194937_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 194937_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146515_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 146515_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235952_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 235952_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194694_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 194694_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 19:59:15.18 +33:06:30.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212950_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 212950_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65661_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 65661_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177172_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 177172_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163673_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 163673_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194017_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 194017_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249908_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 249908_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249679_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 249679_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249575_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 249575_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249553_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 249553_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194339_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 194339_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40441_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 40441_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249382_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 249382_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249369_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 249369_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154890_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 154890_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189805_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 189805_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249249_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 249249_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186717_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 186717_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249196_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 249196_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 19:44:37.08 +28:27:14.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249195_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 249195_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42113_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 42113_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183635_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 183635_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248894_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 248894_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248797_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 248797_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248767_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 248767_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199091_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 199091_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 207858_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 207858_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156760_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 156760_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174606_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 174606_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206242_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 206242_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100617_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 100617_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192877_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 192877_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148747_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 148747_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192697_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 192697_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18995_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 18995_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:27:23.22 +25:09:51.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105461_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 105461_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224725_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 224725_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120438_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 120438_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206079_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 206079_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174611_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 174611_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:32:39.25 +31:33:57.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161317_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 161317_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140919_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 140919_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183368_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 183368_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144058_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 144058_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161805_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 161805_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146263_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 146263_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174965_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 174965_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168387_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 168387_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162655_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 162655_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174602_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 174602_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228886_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 228886_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205727_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 205727_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98392_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 98392_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213319_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 213319_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88836_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 88836_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129210_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 129210_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163919_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 163919_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221757_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 221757_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34302_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 34302_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 230842_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 230842_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73176_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 73176_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157529_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 157529_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151752_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 151752_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156808_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 156808_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109468_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 109468_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128275_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 128275_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202765_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 202765_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227105_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 227105_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 19:26:53.91 +34:07:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110465_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 110465_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227697_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 227697_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251925_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 251925_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106314_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 106314_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181054_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 181054_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 19:30:33.04 +32:50:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153912_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 153912_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18309_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 18309_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:31:19.21 +25:00:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113556_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 113556_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 20:35:09.16 +29:02:33.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178708_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 178708_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89473_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 89473_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225660_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 225660_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159622_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 159622_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131963_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 131963_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213435_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 213435_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125414_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 125414_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21270_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 21270_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216016_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 216016_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91741_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 91741_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107833_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 107833_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212188_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 212188_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113133_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 113133_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197569_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 197569_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92368_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 92368_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198578_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 198578_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175726_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 175726_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216001_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 216001_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232458_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 232458_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178382_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 178382_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168505_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 168505_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178349_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 178349_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215888_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 215888_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156495_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 156495_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 229492_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 229492_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160442_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 160442_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129514_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 129514_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49649_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 49649_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40877_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165
The candidate 40877_fd_Cyg-08-Q1b1x1_2026-05-03_01-57-00_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 215s
Prepared the HTML report for the field Cyg-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:40:03.67 +34:40:51.0
19:41:26.61 +29:34:26.9
19:30:46.58 +29:49:14.3
19:25:51.34 +29:54:15.6
20:07:31.71 +29:35:47.0
19:41:03.44 +30:36:50.4
19:37:07.99 +30:40:26.5
19:48:38.96 +31:02:37.7
19:45:22.21 +31:18:19.0
19:47:16.68 +31:43:23.7
19:49:22.87 +31:50:17.6
19:35:38.77 +31:57:26.1
19:46:23.26 +32:12:45.3
19:26:31.77 +32:34:13.2
20:01:12.06 +32:21:14.6
19:47:46.48 +32:38:46.7
19:39:43.04 +32:53:33.7
19:40:13.26 +32:55:20.3
19:40:14.66 +33:04:03.6
19:35:22.32 +33:24:16.2
19:52:31.81 +33:14:01.8
19:28:27.26 +33:20:37.0
19:50:23.78 +33:15:04.3
19:54:42.55 +33:10:20.8
19:31:11.28 +33:11:46.0
19:54:10.85 +33:02:04.2
19:55:34.35 +32:58:44.2
19:45:44.10 +35:16:36.0
20:06:31.36 +34:31:36.7
19:24:35.82 +34:45:15.5
19:30:57.43 +34:39:45.2
19:40:36.41 +34:20:43.2
19:37:48.66 +34:09:58.0
19:31:55.43 +34:00:57.9
19:50:16.04 +33:51:20.8
19:42:53.61 +33:51:17.6
19:34:29.26 +33:42:34.3
19:25:12.32 +27:08:48.2
19:43:35.56 +31:45:05.4
19:56:15.87 +34:35:55.0
19:46:04.14 +31:28:48.5
19:27:25.76 +35:14:11.6
19:42:15.86 +31:17:50.3
19:52:57.82 +28:27:30.9
19:47:27.71 +25:55:01.4
19:41:36.32 +35:19:38.5
19:50:23.29 +33:14:52.5
20:02:49.55 +33:54:12.0
20:04:48.78 +33:58:38.5
19:44:44.31 +34:09:27.2
19:55:54.94 +31:58:00.4
20:03:02.35 +33:26:28.1
19:59:27.48 +33:21:28.5
20:00:27.78 +32:42:36.0
19:33:29.89 +31:31:18.1
20:10:43.28 +34:52:50.1
19:37:51.32 +32:24:52.5
20:00:21.27 +33:16:03.9
20:02:32.03 +32:08:41.0
20:15:52.48 +30:07:55.9
19:30:08.69 +34:48:09.9
20:00:20.71 +33:16:06.5
19:40:43.03 +33:21:18.7
19:40:14.20 +31:03:20.4
19:25:11.19 +33:10:48.8
19:57:33.29 +30:53:08.2
19:44:57.50 +31:47:37.6
19:59:44.30 +33:03:06.7
19:41:15.87 +29:13:42.4
19:35:45.00 +32:27:29.6
19:54:14.03 +31:50:02.8
20:02:27.45 +34:49:56.1
20:04:10.74 +31:07:40.0
19:45:21.63 +31:17:58.1
19:47:01.69 +31:27:52.3
19:40:32.05 +31:52:33.9
19:54:25.63 +32:29:27.4
19:39:19.71 +31:43:55.2
19:47:38.21 +33:23:46.1
20:18:27.52 +34:37:04.8
19:43:13.55 +35:15:10.9
19:52:29.17 +33:57:52.8
20:02:26.49 +31:38:59.2
19:34:57.89 +33:20:34.4
20:05:27.47 +32:02:22.4
19:35:33.30 +31:52:58.2
19:45:12.45 +29:19:15.7
20:11:29.17 +31:19:33.1
20:10:46.93 +31:55:58.2
19:51:46.86 +32:59:02.6
19:41:58.17 +32:41:21.4
19:47:53.16 +32:44:19.0
19:27:05.70 +29:31:37.5
19:59:44.12 +32:36:58.6
19:31:59.16 +27:32:26.7
19:45:32.60 +28:21:27.1
19:48:27.49 +28:26:19.9
########### Completed Cyg-08-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
19:40:03.67 +34:40:51.0
19:47:27.71 +25:55:01.4
19:41:36.32 +35:19:38.5
19:50:23.29 +33:14:52.5
20:02:49.55 +33:54:12.0
20:04:48.78 +33:58:38.5
19:44:44.31 +34:09:27.2
19:55:54.94 +31:58:00.4
20:03:02.35 +33:26:28.1
19:59:27.48 +33:21:28.5
20:00:27.78 +32:42:36.0
19:33:29.89 +31:31:18.1
20:10:43.28 +34:52:50.1
19:37:51.32 +32:24:52.5
20:00:21.27 +33:16:03.9
20:02:32.03 +32:08:41.0
20:15:52.48 +30:07:55.9
19:30:08.69 +34:48:09.9
20:00:20.71 +33:16:06.5
19:40:43.03 +33:21:18.7
19:40:14.20 +31:03:20.4
19:25:11.19 +33:10:48.8
19:57:33.29 +30:53:08.2
19:44:57.50 +31:47:37.6
19:59:44.30 +33:03:06.7
19:41:15.87 +29:13:42.4
19:35:45.00 +32:27:29.6
19:54:14.03 +31:50:02.8
20:02:27.45 +34:49:56.1
20:04:10.74 +31:07:40.0
19:45:21.63 +31:17:58.1
19:47:01.69 +31:27:52.3
19:40:32.05 +31:52:33.9
19:54:25.63 +32:29:27.4
19:39:19.71 +31:43:55.2
19:47:38.21 +33:23:46.1
20:18:27.52 +34:37:04.8
19:43:13.55 +35:15:10.9
19:52:29.17 +33:57:52.8
20:02:26.49 +31:38:59.2
19:34:57.89 +33:20:34.4
20:05:27.47 +32:02:22.4
19:35:33.30 +31:52:58.2
19:45:12.45 +29:19:15.7
20:11:29.17 +31:19:33.1
20:10:46.93 +31:55:58.2
19:51:46.86 +32:59:02.6
19:41:58.17 +32:41:21.4
19:47:53.16 +32:44:19.0
19:27:05.70 +29:31:37.5
19:59:44.12 +32:36:58.6
19:52:31.81 +33:14:01.8
19:46:04.14 +31:28:48.5
19:52:57.82 +28:27:30.9
19:50:16.04 +33:51:20.8
19:45:32.60 +28:21:27.1
19:41:03.44 +30:36:50.4
19:54:42.55 +33:10:20.8
19:45:22.21 +31:18:19.0
19:34:29.26 +33:42:34.3
19:28:27.26 +33:20:37.0
19:42:15.86 +31:17:50.3
19:27:25.76 +35:14:11.6
19:50:23.78 +33:15:04.3
19:56:15.87 +34:35:55.0
19:40:14.66 +33:04:03.6
19:43:35.56 +31:45:05.4
19:40:13.26 +32:55:20.3
19:25:12.32 +27:08:48.2
19:55:34.35 +32:58:44.2
19:41:26.61 +29:34:26.9
19:35:22.32 +33:24:16.2
19:35:38.77 +31:57:26.1
19:48:38.96 +31:02:37.7
19:39:43.04 +32:53:33.7
19:26:31.77 +32:34:13.2
19:24:35.82 +34:45:15.5
19:37:07.99 +30:40:26.5
19:40:36.41 +34:20:43.2
19:48:27.49 +28:26:19.9
19:47:16.68 +31:43:23.7
20:07:31.71 +29:35:47.0
19:45:44.10 +35:16:36.0
19:30:46.58 +29:49:14.3
19:47:46.48 +32:38:46.7
19:37:48.66 +34:09:58.0
19:30:57.43 +34:39:45.2
19:25:51.34 +29:54:15.6
20:06:31.36 +34:31:36.7
19:31:11.28 +33:11:46.0
19:54:10.85 +33:02:04.2
20:01:12.06 +32:21:14.6
19:42:53.61 +33:51:17.6
19:46:23.26 +32:12:45.3
19:31:55.43 +34:00:57.9
19:49:22.87 +31:50:17.6
19:31:59.16 +27:32:26.7
###################################################################################
19:40:03.67 +34:40:51.0 -- not an asteroid (will add it to exclusion list)
19:47:27.71 +25:55:01.4 -- not an asteroid (will add it to exclusion list)
19:41:36.32 +35:19:38.5 -- not an asteroid (will add it to exclusion list)
19:50:23.29 +33:14:52.5 -- not an asteroid (will add it to exclusion list)
20:02:49.55 +33:54:12.0 -- not an asteroid (will add it to exclusion list)
20:04:48.78 +33:58:38.5 -- not an asteroid (will add it to exclusion list)
19:44:44.31 +34:09:27.2 -- not an asteroid (will add it to exclusion list)
19:55:54.94 +31:58:00.4 -- not an asteroid (will add it to exclusion list)
20:03:02.35 +33:26:28.1 -- not an asteroid (will add it to exclusion list)
19:59:27.48 +33:21:28.5 -- not an asteroid (will add it to exclusion list)
20:00:27.78 +32:42:36.0 -- not an asteroid (will add it to exclusion list)
19:33:29.89 +31:31:18.1 -- not an asteroid (will add it to exclusion list)
20:10:43.28 +34:52:50.1 -- not an asteroid (will add it to exclusion list)
19:37:51.32 +32:24:52.5 -- not an asteroid (will add it to exclusion list)
20:00:21.27 +33:16:03.9 -- not an asteroid (will add it to exclusion list)
20:02:32.03 +32:08:41.0 -- not an asteroid (will add it to exclusion list)
20:15:52.48 +30:07:55.9 -- not an asteroid (will add it to exclusion list)
19:30:08.69 +34:48:09.9 -- not an asteroid (will add it to exclusion list)
20:00:20.71 +33:16:06.5 -- not an asteroid (will add it to exclusion list)
19:40:43.03 +33:21:18.7 -- not an asteroid (will add it to exclusion list)
19:40:14.20 +31:03:20.4 -- not an asteroid (will add it to exclusion list)
19:25:11.19 +33:10:48.8 -- not an asteroid (will add it to exclusion list)
19:57:33.29 +30:53:08.2 -- not an asteroid (will add it to exclusion list)
19:44:57.50 +31:47:37.6 -- not an asteroid (will add it to exclusion list)
19:59:44.30 +33:03:06.7 -- not an asteroid (will add it to exclusion list)
19:41:15.87 +29:13:42.4 -- not an asteroid (will add it to exclusion list)
19:35:45.00 +32:27:29.6 -- not an asteroid (will add it to exclusion list)
19:54:14.03 +31:50:02.8 -- not an asteroid (will add it to exclusion list)
20:02:27.45 +34:49:56.1 -- not an asteroid (will add it to exclusion list)
20:04:10.74 +31:07:40.0 -- not an asteroid (will add it to exclusion list)
19:45:21.63 +31:17:58.1 -- not an asteroid (will add it to exclusion list)
19:47:01.69 +31:27:52.3 -- not an asteroid (will add it to exclusion list)
19:40:32.05 +31:52:33.9 -- not an asteroid (will add it to exclusion list)
19:54:25.63 +32:29:27.4 -- not an asteroid (will add it to exclusion list)
19:39:19.71 +31:43:55.2 -- not an asteroid (will add it to exclusion list)
19:47:38.21 +33:23:46.1 -- not an asteroid (will add it to exclusion list)
20:18:27.52 +34:37:04.8 -- not an asteroid (will add it to exclusion list)
19:43:13.55 +35:15:10.9 -- not an asteroid (will add it to exclusion list)
19:52:29.17 +33:57:52.8 -- not an asteroid (will add it to exclusion list)
20:02:26.49 +31:38:59.2 -- not an asteroid (will add it to exclusion list)
19:34:57.89 +33:20:34.4 -- not an asteroid (will add it to exclusion list)
20:05:27.47 +32:02:22.4 -- not an asteroid (will add it to exclusion list)
19:35:33.30 +31:52:58.2 -- not an asteroid (will add it to exclusion list)
19:45:12.45 +29:19:15.7 -- not an asteroid (will add it to exclusion list)
20:11:29.17 +31:19:33.1 -- not an asteroid (will add it to exclusion list)
20:10:46.93 +31:55:58.2 -- not an asteroid (will add it to exclusion list)
19:51:46.86 +32:59:02.6 -- not an asteroid (will add it to exclusion list)
19:41:58.17 +32:41:21.4 -- not an asteroid (will add it to exclusion list)
19:47:53.16 +32:44:19.0 -- not an asteroid (will add it to exclusion list)
19:27:05.70 +29:31:37.5 -- not an asteroid (will add it to exclusion list)
19:59:44.12 +32:36:58.6 -- not an asteroid (will add it to exclusion list)
19:52:31.81 +33:14:01.8 -- not an asteroid (will add it to exclusion list)
19:46:04.14 +31:28:48.5 -- not an asteroid (will add it to exclusion list)
19:52:57.82 +28:27:30.9 -- not an asteroid (will add it to exclusion list)
19:50:16.04 +33:51:20.8 -- not an asteroid (will add it to exclusion list)
19:45:32.60 +28:21:27.1 -- not an asteroid (will add it to exclusion list)
19:41:03.44 +30:36:50.4 -- not an asteroid (will add it to exclusion list)
19:54:42.55 +33:10:20.8 -- not an asteroid (will add it to exclusion list)
19:45:22.21 +31:18:19.0 -- not an asteroid (will add it to exclusion list)
19:34:29.26 +33:42:34.3 -- not an asteroid (will add it to exclusion list)
19:28:27.26 +33:20:37.0 -- not an asteroid (will add it to exclusion list)
19:42:15.86 +31:17:50.3 -- not an asteroid (will add it to exclusion list)
19:27:25.76 +35:14:11.6 -- not an asteroid (will add it to exclusion list)
19:50:23.78 +33:15:04.3 -- not an asteroid (will add it to exclusion list)
19:56:15.87 +34:35:55.0 -- not an asteroid (will add it to exclusion list)
19:40:14.66 +33:04:03.6 -- not an asteroid (will add it to exclusion list)
19:43:35.56 +31:45:05.4 -- not an asteroid (will add it to exclusion list)
19:40:13.26 +32:55:20.3 -- not an asteroid (will add it to exclusion list)
19:25:12.32 +27:08:48.2 -- not an asteroid (will add it to exclusion list)
19:55:34.35 +32:58:44.2 -- not an asteroid (will add it to exclusion list)
19:41:26.61 +29:34:26.9 -- not an asteroid (will add it to exclusion list)
19:35:22.32 +33:24:16.2 -- not an asteroid (will add it to exclusion list)
19:35:38.77 +31:57:26.1 -- not an asteroid (will add it to exclusion list)
19:48:38.96 +31:02:37.7 -- not an asteroid (will add it to exclusion list)
19:39:43.04 +32:53:33.7 -- not an asteroid (will add it to exclusion list)
19:26:31.77 +32:34:13.2 -- not an asteroid (will add it to exclusion list)
19:24:35.82 +34:45:15.5 -- not an asteroid (will add it to exclusion list)
19:37:07.99 +30:40:26.5 -- not an asteroid (will add it to exclusion list)
19:40:36.41 +34:20:43.2 -- not an asteroid (will add it to exclusion list)
19:48:27.49 +28:26:19.9 -- not an asteroid (will add it to exclusion list)
19:47:16.68 +31:43:23.7 -- not an asteroid (will add it to exclusion list)
20:07:31.71 +29:35:47.0 -- not an asteroid (will add it to exclusion list)
19:45:44.10 +35:16:36.0 -- not an asteroid (will add it to exclusion list)
19:30:46.58 +29:49:14.3 -- not an asteroid (will add it to exclusion list)
19:47:46.48 +32:38:46.7 -- not an asteroid (will add it to exclusion list)
19:37:48.66 +34:09:58.0 -- not an asteroid (will add it to exclusion list)
19:30:57.43 +34:39:45.2 -- not an asteroid (will add it to exclusion list)
19:25:51.34 +29:54:15.6 -- not an asteroid (will add it to exclusion list)
20:06:31.36 +34:31:36.7 -- not an asteroid (will add it to exclusion list)
19:31:11.28 +33:11:46.0 -- not an asteroid (will add it to exclusion list)
19:54:10.85 +33:02:04.2 -- not an asteroid (will add it to exclusion list)
20:01:12.06 +32:21:14.6 -- not an asteroid (will add it to exclusion list)
19:42:53.61 +33:51:17.6 -- not an asteroid (will add it to exclusion list)
19:46:23.26 +32:12:45.3 -- not an asteroid (will add it to exclusion list)
19:31:55.43 +34:00:57.9 -- not an asteroid (will add it to exclusion list)
19:49:22.87 +31:50:17.6 -- not an asteroid (will add it to exclusion list)
19:31:59.16 +27:32:26.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:24:35.82 +34:45:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:11.19 +33:10:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:12.32 +27:08:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:51.34 +29:54:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:31.77 +32:34:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:05.70 +29:31:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:25.76 +35:14:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:28:27.26 +33:20:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:08.69 +34:48:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:46.58 +29:49:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:57.43 +34:39:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:11.28 +33:11:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:55.43 +34:00:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:59.16 +27:32:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:29.89 +31:31:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:29.26 +33:42:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:57.89 +33:20:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:22.32 +33:24:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:33.30 +31:52:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:38.77 +31:57:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:45.00 +32:27:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:07.99 +30:40:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:48.66 +34:09:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:51.32 +32:24:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:19.71 +31:43:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:43.04 +32:53:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:03.67 +34:40:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:13.26 +32:55:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:14.20 +31:03:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:14.66 +33:04:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:32.05 +31:52:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:36.41 +34:20:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:43.03 +33:21:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:03.44 +30:36:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:15.87 +29:13:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:26.61 +29:34:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:36.32 +35:19:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:58.17 +32:41:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:15.86 +31:17:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:53.61 +33:51:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:13.55 +35:15:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:35.56 +31:45:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:44.31 +34:09:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:57.50 +31:47:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:12.45 +29:19:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:21.63 +31:17:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:22.21 +31:18:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:32.60 +28:21:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:44.10 +35:16:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:04.14 +31:28:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:23.26 +32:12:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:01.69 +31:27:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:16.68 +31:43:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:27.71 +25:55:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:38.21 +33:23:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:46.48 +32:38:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:53.16 +32:44:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:27.49 +28:26:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:38.96 +31:02:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:22.87 +31:50:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:16.04 +33:51:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:23.29 +33:14:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:23.78 +33:15:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:46.86 +32:59:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:29.17 +33:57:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:31.81 +33:14:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:57.82 +28:27:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:10.85 +33:02:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:14.03 +31:50:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:25.63 +32:29:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:42.55 +33:10:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:34.35 +32:58:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:54.94 +31:58:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:15.87 +34:35:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:33.29 +30:53:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:27.48 +33:21:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:44.12 +32:36:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:44.30 +33:03:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:20.71 +33:16:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:21.27 +33:16:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:27.78 +32:42:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:12.06 +32:21:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:26.49 +31:38:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:27.45 +34:49:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:32.03 +32:08:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:49.55 +33:54:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:02.35 +33:26:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:10.74 +31:07:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:48.78 +33:58:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:27.47 +32:02:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:31.36 +34:31:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:31.71 +29:35:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:43.28 +34:52:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:46.93 +31:55:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:29.17 +31:19:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:52.48 +30:07:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:27.52 +34:37:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
19:24:35.82 +34:45:15.5 -- not a known variable star
19:25:11.19 +33:10:48.8 -- not a known variable star
19:25:12.32 +27:08:48.2 -- not a known variable star
19:25:51.34 +29:54:15.6 -- not a known variable star
19:26:31.77 +32:34:13.2 -- not a known variable star
19:27:05.70 +29:31:37.5 -- not a known variable star
19:27:25.76 +35:14:11.6 -- not a known variable star
19:28:27.26 +33:20:37.0 -- not a known variable star
19:30:08.69 +34:48:09.9 -- not a known variable star
19:30:46.58 +29:49:14.3 -- not a known variable star
19:30:57.43 +34:39:45.2 -- not a known variable star
19:31:11.28 +33:11:46.0 -- not a known variable star
19:31:55.43 +34:00:57.9 -- a known variable star
19:31:59.16 +27:32:26.7 -- not a known variable star
19:33:29.89 +31:31:18.1 -- a known variable star
19:34:29.26 +33:42:34.3 -- not a known variable star
19:34:57.89 +33:20:34.4 -- a known variable star
19:35:22.32 +33:24:16.2 -- not a known variable star
19:35:33.30 +31:52:58.2 -- not a known variable star
19:35:38.77 +31:57:26.1 -- not a known variable star
19:35:45.00 +32:27:29.6 -- not a known variable star
19:37:07.99 +30:40:26.5 -- not a known variable star
19:37:48.66 +34:09:58.0 -- not a known variable star
19:37:51.32 +32:24:52.5 -- a known variable star
19:39:19.71 +31:43:55.2 -- not a known variable star
19:39:43.04 +32:53:33.7 -- not a known variable star
19:40:03.67 +34:40:51.0 -- a known variable star
19:40:13.26 +32:55:20.3 -- not a known variable star
19:40:14.20 +31:03:20.4 -- not a known variable star
19:40:14.66 +33:04:03.6 -- not a known variable star
19:40:32.05 +31:52:33.9 -- not a known variable star
19:40:36.41 +34:20:43.2 -- not a known variable star
19:40:43.03 +33:21:18.7 -- a known variable star
19:41:03.44 +30:36:50.4 -- not a known variable star
19:41:15.87 +29:13:42.4 -- not a known variable star
19:41:26.61 +29:34:26.9 -- a known variable star
19:41:36.32 +35:19:38.5 -- not a known variable star
19:41:58.17 +32:41:21.4 -- not a known variable star
19:42:15.86 +31:17:50.3 -- not a known variable star
19:42:53.61 +33:51:17.6 -- not a known variable star
19:43:13.55 +35:15:10.9 -- not a known variable star
19:43:35.56 +31:45:05.4 -- not a known variable star
19:44:44.31 +34:09:27.2 -- a known variable star
19:44:57.50 +31:47:37.6 -- not a known variable star
19:45:12.45 +29:19:15.7 -- a known variable star
19:45:21.63 +31:17:58.1 -- a known variable star
19:45:22.21 +31:18:19.0 -- not a known variable star
19:45:32.60 +28:21:27.1 -- a known variable star
19:45:44.10 +35:16:36.0 -- a known variable star
19:46:04.14 +31:28:48.5 -- not a known variable star
19:46:23.26 +32:12:45.3 -- not a known variable star
19:47:01.69 +31:27:52.3 -- not a known variable star
19:47:16.68 +31:43:23.7 -- a known variable star
19:47:27.71 +25:55:01.4 -- not a known variable star
19:47:38.21 +33:23:46.1 -- not a known variable star
19:47:46.48 +32:38:46.7 -- a known variable star
19:47:53.16 +32:44:19.0 -- not a known variable star
19:48:27.49 +28:26:19.9 -- a known variable star
19:48:38.96 +31:02:37.7 -- not a known variable star
19:49:22.87 +31:50:17.6 -- a known variable star
19:50:16.04 +33:51:20.8 -- not a known variable star
19:50:23.29 +33:14:52.5 -- not a known variable star
19:50:23.78 +33:15:04.3 -- a known variable star
19:51:46.86 +32:59:02.6 -- not a known variable star
19:52:29.17 +33:57:52.8 -- not a known variable star
19:52:31.81 +33:14:01.8 -- not a known variable star
19:52:57.82 +28:27:30.9 -- a known variable star
19:54:10.85 +33:02:04.2 -- not a known variable star
19:54:14.03 +31:50:02.8 -- not a known variable star
19:54:25.63 +32:29:27.4 -- not a known variable star
19:54:42.55 +33:10:20.8 -- a known variable star
19:55:34.35 +32:58:44.2 -- a known variable star
19:55:54.94 +31:58:00.4 -- not a known variable star
19:56:15.87 +34:35:55.0 -- a known variable star
19:57:33.29 +30:53:08.2 -- not a known variable star
19:59:27.48 +33:21:28.5 -- a known variable star
19:59:44.12 +32:36:58.6 -- not a known variable star
19:59:44.30 +33:03:06.7 -- a known variable star
20:00:20.71 +33:16:06.5 -- not a known variable star
20:00:21.27 +33:16:03.9 -- not a known variable star
20:00:27.78 +32:42:36.0 -- a known variable star
20:01:12.06 +32:21:14.6 -- a known variable star
20:02:26.49 +31:38:59.2 -- a known variable star
20:02:27.45 +34:49:56.1 -- not a known variable star
20:02:32.03 +32:08:41.0 -- not a known variable star
20:02:49.55 +33:54:12.0 -- not a known variable star
20:03:02.35 +33:26:28.1 -- not a known variable star
20:04:10.74 +31:07:40.0 -- a known variable star
20:04:48.78 +33:58:38.5 -- not a known variable star
20:05:27.47 +32:02:22.4 -- not a known variable star
20:06:31.36 +34:31:36.7 -- not a known variable star
20:07:31.71 +29:35:47.0 -- not a known variable star
20:10:43.28 +34:52:50.1 -- not a known variable star
20:10:46.93 +31:55:58.2 -- not a known variable star
20:11:29.17 +31:19:33.1 -- not a known variable star
20:15:52.48 +30:07:55.9 -- not a known variable star
20:18:27.52 +34:37:04.8 -- not a known variable star
Found 70 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
97 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 97 (excluding asteroids and hot pixels, 70 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461163.78902543 -observatory V36
01:53:49.05 +09:54:18.6 Mercury (-1.0mag)
04:35:45.97 +23:01:55.0 Venus (-3.9mag)
01:06:49.78 +06:09:39.5 Mars (1.2mag)
07:21:57.40 +22:29:44.4 Jupiter (-2.0mag)
00:36:37.42 +01:34:41.9 Saturn (0.9mag)
03:51:33.54 +19:59:38.3 Uranus (5.8mag)
00:12:58.07 -00:02:06.3 Neptune (7.8mag)
20:34:13.07 -22:54:28.7 Pluto (14.5mag)
15:46:45.85 -25:44:41.4 Moon (-12.3mag)
-rw-r--r-- 1 apache apache 363 May 3 01:59 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461163.78902543:
07:21:50.64 +22:29:59.5 Io (5.9mag)
07:21:50.97 +22:30:01.8 Europa (6.0mag)
07:21:39.25 +22:30:25.7 Ganymede (5.4mag)
07:22:31.08 +22:28:26.5 Callisto (6.7mag)
07:24:24.72 +22:10:35.6 Himalia (15.4mag)
07:21:58.93 +22:29:42.5 Thebe (16.3mag)
07:24:51.66 +22:39:35.0 Elara (17.4mag)
07:21:59.88 +23:00:41.0 Pasiphae (17.5mag)
07:29:50.61 +22:29:09.3 Carme (18.6mag)
00:36:33.26 +01:35:10.7 Titan (8.7mag)
00:36:34.07 +01:34:55.3 Rhea (10.0mag)
00:36:11.34 +01:32:41.7 Iapetus (11.5mag)
00:36:52.69 +01:34:35.9 Hyperion (14.8mag)
00:37:59.14 +01:41:29.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 3 01:59 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461163.78902543:
16:38:35.42 -26:03:51.1 JWST
18:02:10.62 +34:53:13.9 Chandra
18:47:46.85 -19:00:01.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 3 01:59 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461163.78902543 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
06:43:18.44 +29:14:04.5 17.8mag P/2009 WX51 (Catalina)
18:55:53.39 -29:54:20.3 13.8mag P/2010 H2 (Vales)
05:20:17.25 -68:55:53.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:36:53.34 +31:34:25.1 17.3mag C/2017 K2 (PANSTARRS)
17:27:19.45 +12:29:21.1 17.7mag C/2021 G2 (ATLAS)
23:13:44.56 +29:58:51.4 17.1mag C/2022 E2 (ATLAS)
04:49:52.06 +26:27:52.8 16.2mag C/2022 N2 (PANSTARRS)
09:08:56.00 +31:57:33.1 16.4mag C/2022 QE78 (ATLAS)
08:35:05.95 +01:30:54.8 17.4mag C/2022 R6 (PANSTARRS)
18:48:03.09 +19:53:10.4 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:34:11.26 -11:16:18.2 17.5mag P/2023 B1 (PANSTARRS)
09:01:47.77 -09:19:57.0 17.8mag C/2023 F3 (ATLAS)
22:08:18.00 +64:01:31.0 17.6mag C/2023 H5 (Lemmon)
18:59:19.25 -04:11:56.4 13.9mag C/2023 R1 (PANSTARRS)
19:16:00.95 +88:08:10.2 17.9mag C/2023 X2 (Lemmon)
06:29:30.06 +63:32:47.2 17.3mag C/2024 A1 (ATLAS)
05:47:29.01 +22:51:07.6 12.1mag C/2024 E1 (Wierzchos)
16:06:46.99 +09:08:00.7 17.3mag C/2024 G6 (ATLAS)
20:23:34.84 +20:11:47.3 14.4mag C/2024 J3 (ATLAS)
03:42:28.49 -19:55:27.1 16.2mag C/2024 T5 (ATLAS)
05:32:07.72 +41:19:33.1 17.8mag C/2025 J1 (Borisov)
12:34:10.98 +52:09:29.5 16.0mag C/2025 L1 (ATLAS)
03:54:44.44 -29:12:06.4 18.0mag C/2025 Q3 (ATLAS)
04:25:43.30 -02:26:33.1 8.8mag C/2025 R3 (PANSTARRS)
12:47:08.77 +03:55:48.1 17.3mag C/2025 Y1 (ATLAS)
05:00:33.81 +01:38:35.3 16.8mag C/2026 A1 (MAPS)
00:45:17.50 +39:54:37.4 15.1mag C/2026 B2 (Sun-Gao)
19:16:20.87 -08:47:28.8 10.8mag 10P/Tempel
14:37:38.52 +01:01:09.2 15.6mag 24P/Schaumasse
10:59:34.52 -01:04:29.3 15.8mag 29P/Schwassmann-Wachmann
10:39:59.47 -03:01:49.3 17.3mag 43P/Wolf-Harrington
02:15:36.02 +20:20:49.8 17.4mag 47P/Ashbrook-Jackson
07:44:27.84 +33:07:24.6 16.9mag 63P/Wild
23:50:09.52 -09:29:25.3 15.7mag 65P/Gunn
04:51:40.42 +26:36:20.7 16.1mag 76P/West-Kohoutek-Ikemura
01:44:29.50 +11:31:18.9 14.1mag 78P/Gehrels
23:52:43.43 -04:19:41.5 14.9mag 88P/Howell
03:01:09.06 +24:51:56.9 15.0mag 93P/Lovas
05:29:22.36 +33:01:58.9 16.0mag 123P/West-Hartley
08:51:37.94 +30:27:09.8 16.3mag 124P/Mrkos
03:00:26.35 +16:12:22.6 16.4mag 128P/Shoemaker-Holt
03:21:45.64 +16:25:10.2 17.6mag 131P/Mueller
02:59:26.55 +17:55:54.2 10.8mag 141P/Machholz
03:05:13.61 +10:58:17.2 10.8mag 141P-A/Machholz
01:45:20.68 +06:48:09.3 11.0mag 141P-D/Machholz
01:51:21.55 +07:12:06.3 14.9mag 162P/SidingSpring
22:23:42.77 -07:26:49.1 18.0mag 218P/LINEAR
17:15:45.01 -11:48:37.0 16.1mag 235P/LINEAR
06:12:48.36 +35:38:57.0 17.0mag 240P/NEAT
07:48:39.60 -03:31:22.1 17.9mag 242P/Spahr
23:00:17.62 -15:54:19.8 17.4mag 260P/McNaught
02:35:12.64 +24:43:22.8 17.8mag 295P/LINEAR
15:34:28.39 +07:55:59.2 17.4mag 391P/Kowalski
07:42:25.14 +21:19:58.9 17.7mag 450P/LONEOS
06:02:06.34 +44:01:03.5 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K May 3 01:59 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
21:00:10.71 -32:17:03.90 2026-04-27.36 16.15
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:00:10.71 -32:17:03.90 2026-04-27.36 16.15
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
-rw-r--r-- 1 apache apache 5.8K May 3 01:59 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
-rw-r--r-- 1 apache apache 188K May 3 01:59 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:10:53.458 +45:56:52.48 SN 2026knu 2026-04-20.18 19.5784
13:23:31.702 -27:27:16.87 AT 2026knt 2026-04-21.45 19.6
14:59:13.174 -10:47:02.79 AT 2026kns 2026-04-09.59 20.1
14:45:20.668 -24:47:31.93 AT 2026knr 2026-03-24.65 20.36
11:45:24.981 +14:40:44.45 AT 2026knq 2026-04-13.92 20.18
04:52:30.865 -15:17:09.10 AT 2026knp 2026-04-20.71 18.098
17:25:02.776 +69:43:35.23 AT 2026kno 2026-04-23.10 19.208
15:15:42.943 -39:27:45.41 AT 2026knn 2026-04-14.63 19.62
21:02:34.025 +19:12:44.83 AT 2026knm 2026-04-22.60 18.74
14:38:36.298 -39:37:27.88 AT 2026knl 2026-04-21.52 20.1
13:24:43.943 +16:55:43.96 AT 2026knk 2026-04-20.96 20.03
13:55:11.417 +21:19:35.16 AT 2026knj 2026-04-20.98 19.3
16:21:58.180 +07:39:22.34 AT 2026kni 2026-04-22.11 19.97
18:25:00.619 +56:31:13.17 AT 2026knh 2026-04-14.18 19.89
11:52:14.846 +19:25:04.67 AT 2026kng 2026-04-12.92 20.24
17:52:14.690 -78:03:43.36 AT 2026kne 2026-04-23.29 18.712
19:46:54.481 -51:39:39.32 AT 2026knd 2026-04-20.32 17.94
21:24:26.061 +26:56:11.62 AT 2026knc 2026-04-23.59 17.66
11:18:30.556 -08:06:31.77 AT 2026knb 2026-04-22.86 19.129
14:56:59.281 +45:09:43.33 AT 2026kna 2026-04-23.01 19.329
-rw-r--r-- 1 apache apache 30K May 3 01:59 tns_transients_list.txt
