This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9
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 11 04.1803 2461348.6803 13.98 19:26:25.48 +22:35:58.4
56.91968 2.88229 galactic Vul Second-epoch detections are separated by 2.0" and 7.5 pix
The object was found in VSX 4" NSVS 11225566
Type: SR
# Max. Min./Amp. JD0 Period
15.223 r Y 0.450 r 2451353.30000 109.582170700000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:26:25.48 +22:35:58.4: 15.42 +/- 0.20 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:26:25.48 +22:35:58.4: 15.54 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.48 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11225566,2461348.6803,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11225566 20261104.1803 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.13 18:54:24.04 +23:33:16.1
54.43198 9.88518 galactic Her Second-epoch detections are separated by 6.4" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:54:24.04 +23:33:16.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:54:24.04 +23:33:16.1: 14.10 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:54:24.04 +23:33:16.1: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 54 24.04 +23 33 16.1 13.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461348.6803,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261104.1803 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.40 18:58:45.23 +25:27:15.4
56.60493 9.80700 galactic Vul Second-epoch detections are separated by 0.6" and 7.5 pix
The object was found in VSX 4" NSVS 8204043
Type: SR
# Max. Min./Amp. JD0 Period
14.879 g Y 1.042 g 2458200.09330 323.133065000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:58:45.23 +25:27:15.4: 12.61 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:58:45.23 +25:27:15.4: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8204043,2461348.6803,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8204043 20261104.1803 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.08 19:19:27.87 +24:26:21.3
57.80136 5.15302 galactic Vul Second-epoch detections are separated by 4.3" and 7.0 pix
The object was found in VSX 4" ASASSN-V J191927.61+242621.1
Type: SR
# Max. Min./Amp. JD0 Period
15.000 V 15.500 V 2458300.88610 241.665942300000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:19:27.87 +24:26:21.3: 14.06 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:19:27.87 +24:26:21.3: 14.09 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191927.61+242621.1,2461348.6803,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191927.61+242621.1 20261104.1803 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.32 19:39:17.76 +18:21:34.8
54.66168 -1.80409 galactic Sge Second-epoch detections are separated by 3.1" and 7.6 pix
The object was found in VSX 4" Mis V0987
Type: M
# Max. Min./Amp. JD0 Period
18.773 g Y 4.044 g 2458520.30540 401.604263600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:39:17.76 +18:21:34.8: 14.30 +/- 0.11 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:39:17.76 +18:21:34.8: 14.61 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V0987,2461348.6803,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0987 20261104.1803 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.38 19:52:13.65 +26:35:19.1
63.27921 -0.26026 galactic Vul Second-epoch detections are separated by 1.3" and 6.9 pix
The object was found in VSX 8" ZTF J195214.02+263525.0
Type: SR
# Max. Min./Amp. JD0 Period
14.399 r Y 0.154 r 2458311.85040 78.973044300000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:52:13.65 +26:35:19.1: 14.91 +/- 0.18 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:52:13.65 +26:35:19.1: 14.90 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195214.02+263525.0,2461348.6803,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195214.02+263525.0 20261104.1803 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.74 19:27:43.61 +26:08:30.5
60.18717 4.29698 galactic Vul Second-epoch detections are separated by 1.0" and 7.0 pix
The object was found in VSX 4" ASASSN-V J192743.69+260834.1
Type: SR
# Max. Min./Amp. JD0 Period
15.520 g Y 0.530 g 2459473.78200 494.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:27:43.61 +26:08:30.5: 14.72 +/- 0.15 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:27:43.61 +26:08:30.5: 14.73 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192743.69+260834.1,2461348.6803,13.74,0.05,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
ASASSN-V J192743.69+260834.1 20261104.1803 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.64 19:26:16.91 +18:00:18.5
52.85766 0.73097 galactic Sge Second-epoch detections are separated by 3.4" and 6.8 pix
The object was found in VSX 5" ZTF J192616.57+180018.1
Type: SR
# Max. Min./Amp. JD0 Period
15.551 r Y 0.558 r 2458382.13000 230.682208200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:26:16.91 +18:00:18.5: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:26:16.91 +18:00:18.5: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192616.57+180018.1,2461348.6803,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192616.57+180018.1 20261104.1803 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.99 19:26:05.19 +17:26:57.3
52.34644 0.50769 galactic Sge Second-epoch detections are separated by 3.3" and 7.8 pix
The object was found in VSX 2" ZTF J192605.20+172659.3
Type: SR
# Max. Min./Amp. JD0 Period
14.461 r Y 0.090 r 2458327.78710 24.323503500000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:26:05.19 +17:26:57.3: 15.13 +/- 0.17 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:26:05.19 +17:26:57.3: 15.37 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.22 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192605.20+172659.3,2461348.6803,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192605.20+172659.3 20261104.1803 13.99CV 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 11 04.1803 2461348.6803 13.86 19:33:24.58 +24:18:23.9
59.18715 2.29129 galactic Vul Second-epoch detections are separated by 1.5" and 7.3 pix
The object was found in VSX 4" ASASSN-V J193324.84+241825.0
Type: L:
# Max. Min./Amp. JD0 Period
15.500 V 16.100 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:33:24.58 +24:18:23.9: 15.17 +/- 0.23 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:33:24.58 +24:18:23.9: 15.30 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.22 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J193324.84+241825.0,2461348.6803,13.86,0.05,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
ASASSN-V J193324.84+241825.0 20261104.1803 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.55 19:21:43.99 +24:02:05.0
57.68241 4.50722 galactic Vul Second-epoch detections are separated by 0.4" and 7.1 pix
The object was found in VSX 4" ASASSN-V J192143.77+240207.1
Type: SR
# Max. Min./Amp. JD0 Period
14.600 V 15.700 V 2457668.80000 347.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:21:43.99 +24:02:05.0: 13.82 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:21:43.99 +24:02:05.0: 13.79 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192143.77+240207.1,2461348.6803,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192143.77+240207.1 20261104.1803 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.87 19:32:37.28 +23:50:58.9
58.69969 2.22859 galactic Vul Second-epoch detections are separated by 1.5" and 6.9 pix
The object was found in VSX 2" ASASSN-V J193237.30+235100.4
Type: SR
# Max. Min./Amp. JD0 Period
15.579 g Y 0.674 g 2458317.23220 70.801999200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:32:37.28 +23:50:58.9: 13.87 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:32:37.28 +23:50:58.9: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193237.30+235100.4,2461348.6803,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193237.30+235100.4 20261104.1803 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.63 19:01:00.32 +18:41:45.8
50.70180 6.37193 galactic Sge Second-epoch detections are separated by 1.9" and 7.5 pix
The object was found in VSX 8" ASASSN-V J190059.84+184150.3
Type: SR
# Max. Min./Amp. JD0 Period
14.160 V 14.410 V 2457167.90000 58.760000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:01:00.32 +18:41:45.8: 13.67 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:01:00.32 +18:41:45.8: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190059.84+184150.3,2461348.6803,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190059.84+184150.3 20261104.1803 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.92 19:21:09.98 +26:31:01.9
59.83102 5.77206 galactic Vul Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 2" ASASSN-V J192110.01+263103.4
Type: SR
# Max. Min./Amp. JD0 Period
15.901 g Y 0.568 g 2458647.50500 270.372340000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:21:09.98 +26:31:01.9: 13.98 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:21:09.98 +26:31:01.9: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192110.01+263103.4,2461348.6803,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192110.01+263103.4 20261104.1803 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.53 19:27:18.11 +22:21:35.6
56.80465 2.59023 galactic Vul Second-epoch detections are separated by 2.0" and 7.4 pix
The object was found in VSX 2" Gaia DR3 2018999499514435840
Type: SR|M
# Max. Min./Amp. JD0 Period
12.530 G 13.220 G 438.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:27:18.11 +22:21:35.6: 14.78 +/- 0.12 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:27:18.11 +22:21:35.6: 14.73 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.75 +/- 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 2018999499514435840,2461348.6803,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2018999499514435840 20261104.1803 13.53CV 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 11 04.1803 2461348.6803 11.67 18:57:56.52 +21:21:20.1
52.78510 8.19420 galactic Vul Second-epoch detections are separated by 0.2" and 7.4 pix
The object was found in VSX 4" ASASSN-V J185756.40+212116.0
Type: L:
# Max. Min./Amp. JD0 Period
13.260 V 13.830 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:57:56.52 +21:21:20.1: 12.64 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:57:56.52 +21:21:20.1: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185756.40+212116.0,2461348.6803,11.67,0.05,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
ASASSN-V J185756.40+212116.0 20261104.1803 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 11 04.1803 2461348.6803 11.63 19:13:42.11 +23:43:58.1
56.56491 5.99831 galactic Vul Second-epoch detections are separated by 0.8" and 7.5 pix
The object was found in VSX 2" ASASSN-V J191342.09+234359.4
Type: SR
# Max. Min./Amp. JD0 Period
12.790 V 13.150 V 2458639.67160 53.532879000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:13:42.11 +23:43:58.1: 12.67 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:13:42.11 +23:43:58.1: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191342.09+234359.4,2461348.6803,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191342.09+234359.4 20261104.1803 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.06 19:21:02.45 +25:23:42.5
58.81838 5.27822 galactic Vul Second-epoch detections are separated by 0.8" and 7.3 pix
The object was found in VSX 4" ASASSN-V J192102.50+252346.2
Type: SR
# Max. Min./Amp. JD0 Period
14.580 V 14.970 V 2457464.10000 60.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:21:02.45 +25:23:42.5: 14.09 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:21:02.45 +25:23:42.5: 14.08 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192102.50+252346.2,2461348.6803,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192102.50+252346.2 20261104.1803 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.79 19:24:05.92 +23:43:30.8
57.66158 3.88451 galactic Vul Second-epoch detections are separated by 0.2" and 7.2 pix
The object was found in VSX 1" ASASSN-V J192405.96+234331.9
Type: L
# Max. Min./Amp. JD0 Period
13.140 V 13.490 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:24:05.92 +23:43:30.8: 12.70 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:24:05.92 +23:43:30.8: 12.71 +/- 0.02 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
ASASSN-V J192405.96+234331.9,2461348.6803,11.79,0.05,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
ASASSN-V J192405.96+234331.9 20261104.1803 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 11 04.1803 2461348.6803 13.28 19:26:41.80 +24:12:26.7
58.36800 3.58811 galactic Vul Second-epoch detections are separated by 0.7" and 7.1 pix
The object was found in VSX 2" ASASSN-V J192641.90+241228.7
Type: SR
# Max. Min./Amp. JD0 Period
15.750 g Y 0.550 g 2458730.57800 75.780000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:26:41.80 +24:12:26.7: 14.12 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:26:41.80 +24:12:26.7: 14.20 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 J192641.90+241228.7,2461348.6803,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192641.90+241228.7 20261104.1803 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.01 18:56:17.36 +19:28:47.5
50.91191 7.71812 galactic Her Second-epoch detections are separated by 0.4" and 7.5 pix
The object was found in VSX 2" ASASSN-V J185617.21+192846.9
Type: L
# Max. Min./Amp. JD0 Period
13.350 V 13.750 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:56:17.36 +19:28:47.5: 12.92 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:56:17.36 +19:28:47.5: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 56 17.36 +19 28 47.5 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185617.21+192846.9,2461348.6803,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185617.21+192846.9 20261104.1803 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.04 19:15:03.21 +22:56:16.0
55.99615 5.35955 galactic Vul Second-epoch detections are separated by 0.1" and 7.3 pix
The object was found in VSX 2" ASASSN-V J191503.25+225618.2
Type: L:
# Max. Min./Amp. JD0 Period
13.560 V 13.810 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:15:03.21 +22:56:16.0: 12.99 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:15:03.21 +22:56:16.0: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191503.25+225618.2,2461348.6803,12.04,0.05,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
ASASSN-V J191503.25+225618.2 20261104.1803 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 11 04.1803 2461348.6803 12.02 19:10:23.03 +24:24:57.2
56.83386 6.98256 galactic Vul Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 3" ASASSN-V J191022.89+242459.4
Type: SRS
# Max. Min./Amp. JD0 Period
14.550 g Y 0.430 g 2459422.57900 27.219000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:10:23.03 +24:24:57.2: 13.02 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:10:23.03 +24:24:57.2: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191022.89+242459.4,2461348.6803,12.02,0.05,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
ASASSN-V J191022.89+242459.4 20261104.1803 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 11 04.1803 2461348.6803 13.07 19:17:29.53 +24:16:05.4
57.44106 5.47294 galactic Vul Second-epoch detections are separated by 1.1" and 7.0 pix
The object was found in VSX 2" ASASSN-V J191729.55+241607.3
Type: SR
# Max. Min./Amp. JD0 Period
15.910 g Y 0.640 g 2458366.61900 66.060000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:17:29.53 +24:16:05.4: 14.19 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:17:29.53 +24:16:05.4: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191729.55+241607.3,2461348.6803,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191729.55+241607.3 20261104.1803 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.91 19:12:01.63 +24:43:11.1
57.27651 6.78554 galactic Vul Second-epoch detections are separated by 3.2" and 7.1 pix
The object was found in VSX 5" ASASSN-V J191201.50+244315.5
Type: SR
# Max. Min./Amp. JD0 Period
13.290 V 13.730 V 2457471.10000 73.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:01.63 +24:43:11.1: 13.09 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:01.63 +24:43:11.1: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191201.50+244315.5,2461348.6803,11.91,0.05,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
ASASSN-V J191201.50+244315.5 20261104.1803 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 11 04.1803 2461348.6803 12.25 19:45:50.07 +26:44:26.9
62.68648 1.04810 galactic Vul Second-epoch detections are separated by 0.8" and 7.1 pix
The object was found in VSX 3" ASASSN-V J194550.20+264429.0
Type: SR
# Max. Min./Amp. JD0 Period
13.890 V 14.290 V 2458283.88310 67.253787400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:45:50.07 +26:44:26.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:45:50.07 +26:44:26.9: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194550.20+264429.0,2461348.6803,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194550.20+264429.0 20261104.1803 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.34 19:32:51.16 +21:39:03.9
56.79867 1.12132 galactic Vul Second-epoch detections are separated by 2.2" and 7.3 pix
The object was found in VSX 1" ZTF J193251.22+213904.8
Type: SR
# Max. Min./Amp. JD0 Period
13.601 r Y 0.105 r 2458377.76770 39.230476600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:32:51.16 +21:39:03.9: 14.26 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:32:51.16 +21:39:03.9: 14.48 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.35 +/- 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
ZTF J193251.22+213904.8,2461348.6803,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193251.22+213904.8 20261104.1803 13.34CV 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 11 04.1803 2461348.6803 12.03 19:15:37.49 +24:12:07.9
57.18621 5.82115 galactic Vul Second-epoch detections are separated by 1.4" and 7.0 pix
The object was found in VSX 1" NSVS 8343181
Type: L
# Max. Min./Amp. JD0 Period
11.050 R1 11.400 R1
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:15:37.49 +24:12:07.9: 13.23 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:15:37.49 +24:12:07.9: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8343181,2461348.6803,12.03,0.05,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
NSVS 8343181 20261104.1803 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 11 04.1803 2461348.6803 12.18 19:16:00.88 +26:44:19.9
59.49930 6.89720 galactic Lyr Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 3" ASASSN-V J191600.85+264423.0
Type: L:
# Max. Min./Amp. JD0 Period
13.980 V 14.550 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:16:00.88 +26:44:19.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:16:00.88 +26:44:19.9: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191600.85+264423.0,2461348.6803,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191600.85+264423.0 20261104.1803 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.41 19:17:59.97 +22:31:43.0
55.94499 4.56819 galactic Vul Second-epoch detections are separated by 1.2" and 7.5 pix
The object was found in VSX 1" ASASSN-V J191800.02+223143.6
Type: SR
# Max. Min./Amp. JD0 Period
13.840 V 14.020 V 2458027.00000 235.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:17:59.97 +22:31:43.0: 13.22 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:17:59.97 +22:31:43.0: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191800.02+223143.6,2461348.6803,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191800.02+223143.6 20261104.1803 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.31 19:13:02.37 +21:28:55.4
54.48205 5.10856 galactic Vul Second-epoch detections are separated by 1.9" and 7.6 pix
The object was found in VSX 2" ASASSN-V J191302.22+212854.0
Type: SR
# Max. Min./Amp. JD0 Period
14.540 V 14.700 V 2457133.00000 31.610000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:13:02.37 +21:28:55.4: 14.26 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:13:02.37 +21:28:55.4: 14.32 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191302.22+212854.0,2461348.6803,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191302.22+212854.0 20261104.1803 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.39 19:12:49.22 +17:56:29.7
51.30309 3.53065 galactic Sge Second-epoch detections are separated by 1.4" and 7.7 pix
The object was found in VSX 1" ZTF J191249.17+175629.3
Type: SR
# Max. Min./Amp. JD0 Period
16.366 g Y 0.182 g 2458217.98060 56.067337500000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:49.22 +17:56:29.7: 14.34 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:49.22 +17:56:29.7: 14.50 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191249.17+175629.3,2461348.6803,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191249.17+175629.3 20261104.1803 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.41 19:14:52.38 +23:17:46.6
56.29737 5.56038 galactic Vul Second-epoch detections are separated by 0.2" and 7.3 pix
The object was found in VSX 1" ASASSN-V J191452.34+231747.9
Type: SRS
# Max. Min./Amp. JD0 Period
13.820 V 14.020 V 2457065.17000 22.373000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:14:52.38 +23:17:46.6: 13.33 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:14:52.38 +23:17:46.6: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191452.34+231747.9,2461348.6803,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191452.34+231747.9 20261104.1803 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.05 19:36:37.67 +25:17:22.4
60.40182 2.12912 galactic Vul Second-epoch detections are separated by 2.4" and 6.7 pix
The object was found in VSX 4" NSVS J1936377+251728
Type: M
# Max. Min./Amp. JD0 Period
16.719 g Y 3.527 g 2458485.20770 352.676992000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:36:37.67 +25:17:22.4: 14.33 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:36:37.67 +25:17:22.4: 14.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1936377+251728,2461348.6803,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1936377+251728 20261104.1803 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.13 19:23:43.61 +25:03:39.4
58.80515 4.58503 galactic Vul Second-epoch detections are separated by 2.7" and 6.8 pix
The object was found in VSX 5" ASASSN-V J192343.28+250341.2
Type: SR
# Max. Min./Amp. JD0 Period
14.190 V 14.430 V 2458612.45990 54.079288100000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:23:43.61 +25:03:39.4: 14.16 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:23:43.61 +25:03:39.4: 14.16 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192343.28+250341.2,2461348.6803,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192343.28+250341.2 20261104.1803 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.59 19:18:05.50 +24:44:03.7
57.92002 5.56598 galactic Vul Second-epoch detections are separated by 3.1" and 7.2 pix
The object was found in VSX 7" ASASSN-V J191805.00+244401.4
Type: SR
# Max. Min./Amp. JD0 Period
13.980 V 14.220 V 2457855.00000 528.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:18:05.50 +24:44:03.7: 13.50 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:18:05.50 +24:44:03.7: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191805.00+244401.4,2461348.6803,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191805.00+244401.4 20261104.1803 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.62 19:12:48.22 +24:12:51.5
56.90291 6.39959 galactic Vul Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 2" ASASSN-V J191248.16+241252.9
Type: SRS
# Max. Min./Amp. JD0 Period
13.940 V 14.080 V 2457074.16000 19.776000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:48.22 +24:12:51.5: 13.57 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:48.22 +24:12:51.5: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191248.16+241252.9,2461348.6803,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191248.16+241252.9 20261104.1803 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.60 19:23:27.89 +25:05:34.3
58.80564 4.65240 galactic Vul Second-epoch detections are separated by 0.7" and 7.0 pix
The object was found in VSX 3" ZTF J192328.00+250537.3
Type: SR
# Max. Min./Amp. JD0 Period
12.980 r Y 0.212 r 2458608.86430 41.611667000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:23:27.89 +25:05:34.3: 13.62 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:23:27.89 +25:05:34.3: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192328.00+250537.3,2461348.6803,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192328.00+250537.3 20261104.1803 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.33 19:17:59.22 +17:31:47.2
51.50825 2.24957 galactic Sge Second-epoch detections are separated by 1.6" and 7.4 pix
The object was found in VSX 0" ASASSN-V J191759.24+173147.2
Type: SR
# Max. Min./Amp. JD0 Period
16.600 g Y 0.710 g 2458694.64400 475.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:17:59.22 +17:31:47.2: 14.55 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:17:59.22 +17:31:47.2: 14.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.45 +/- 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
ASASSN-V J191759.24+173147.2,2461348.6803,13.33,0.05,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
ASASSN-V J191759.24+173147.2 20261104.1803 13.33CV 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 11 04.1803 2461348.6803 13.04 19:21:40.69 +23:13:37.9
56.96002 4.14202 galactic Vul Second-epoch detections are separated by 3.2" and 7.7 pix
The object was found in VSX 3" ZTF J192140.93+231338.2
Type: SR
# Max. Min./Amp. JD0 Period
13.589 r Y 0.364 r 2458605.51410 190.368979200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:21:40.69 +23:13:37.9: 14.37 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:21:40.69 +23:13:37.9: 14.26 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192140.93+231338.2,2461348.6803,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192140.93+231338.2 20261104.1803 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.40 19:12:07.74 +24:36:54.6
57.19301 6.71774 galactic Vul Second-epoch detections are separated by 1.1" and 7.4 pix
The object was found in VSX 2" Gaia DR3 2023572815032207360
Type: SR|M
# Max. Min./Amp. JD0 Period
12.350 G 12.530 G 39.180000000000 M
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:07.74 +24:36:54.6: 14.55 +/- 0.11 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:07.74 +24:36:54.6: 14.56 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.56 +/- 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 2023572815032207360,2461348.6803,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2023572815032207360 20261104.1803 13.40CV 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 11 04.1803 2461348.6803 12.54 19:04:40.56 +26:45:09.9
58.37524 9.17079 galactic Lyr Second-epoch detections are separated by 1.0" and 7.4 pix
The object was found in VSX 6" ASASSN-V J190440.55+264516.4
Type: L:
# Max. Min./Amp. JD0 Period
13.780 V 14.070 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:40.56 +26:45:09.9: 13.50 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:40.56 +26:45:09.9: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190440.55+264516.4,2461348.6803,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190440.55+264516.4 20261104.1803 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.39 19:11:29.36 +19:39:17.9
52.68462 4.59645 galactic Sge Second-epoch detections are separated by 3.1" and 7.8 pix
The object was found in VSX 1" ZTF J191129.31+193918.6
Type: SR
# Max. Min./Amp. JD0 Period
13.789 r Y 0.136 r 2458389.55620 40.553892300000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:29.36 +19:39:17.9: 14.56 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:29.36 +19:39:17.9: 14.52 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191129.31+193918.6,2461348.6803,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191129.31+193918.6 20261104.1803 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.44 19:10:07.59 +20:53:42.5
53.64679 5.44586 galactic Sge Second-epoch detections are separated by 2.2" and 7.8 pix
The object was found in VSX 1" ASASSN-V J191007.67+205343.5
Type: SR
# Max. Min./Amp. JD0 Period
14.880 V 15.480 V 2457538.00000 64.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:10:07.59 +20:53:42.5: 14.56 +/- 0.11 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:10:07.59 +20:53:42.5: 14.75 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191007.67+205343.5,2461348.6803,13.44,0.05,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
ASASSN-V J191007.67+205343.5 20261104.1803 13.44CV 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 11 04.1803 2461348.6803 12.58 19:11:46.21 +24:43:52.8
57.26044 6.84286 galactic Vul Second-epoch detections are separated by 0.8" and 7.2 pix
The object was found in VSX 8" ASASSN-V J191145.66+244351.4
Type: L:
# Max. Min./Amp. JD0 Period
13.700 V 13.970 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:46.21 +24:43:52.8: 13.45 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:46.21 +24:43:52.8: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191145.66+244351.4,2461348.6803,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191145.66+244351.4 20261104.1803 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.65 18:59:52.04 +21:30:00.8
53.11513 7.85525 galactic Vul Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 5" ASASSN-V J185951.79+213003.7
Type: SR
# Max. Min./Amp. JD0 Period
14.070 V 14.830 V 2457137.00000 48.850000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:59:52.04 +21:30:00.8: 13.68 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:59:52.04 +21:30:00.8: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185951.79+213003.7,2461348.6803,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185951.79+213003.7 20261104.1803 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.47 19:35:38.44 +18:13:38.0
54.12182 -1.11192 galactic Sge Second-epoch detections are separated by 1.6" and 7.6 pix
The object was found in VSX 3" NSVS 11252248
Type: SR
# Max. Min./Amp. JD0 Period
13.149 r Y 0.300 R1 2458343.39910 181.145303900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:35:38.44 +18:13:38.0: 13.46 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:35:38.44 +18:13:38.0: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11252248,2461348.6803,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11252248 20261104.1803 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.55 19:03:17.58 +20:03:09.5
52.16572 6.49534 galactic Sge Second-epoch detections are separated by 1.1" and 7.3 pix
The object was found in VSX 2" ASASSN-V J190317.46+200309.8
Type: SR
# Max. Min./Amp. JD0 Period
14.010 V 14.470 V 2458651.94170 80.077191300000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:03:17.58 +20:03:09.5: 13.67 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:03:17.58 +20:03:09.5: 13.70 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190317.46+200309.8,2461348.6803,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190317.46+200309.8 20261104.1803 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.57 18:57:38.82 +23:40:46.4
54.87143 9.26806 galactic Vul Second-epoch detections are separated by 1.3" and 7.3 pix
The object was found in VSX 4" ASASSN-V J185738.73+234050.0
Type: SR
# Max. Min./Amp. JD0 Period
14.090 V 14.460 V 2458273.53930 167.423743200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:57:38.82 +23:40:46.4: 13.67 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:57:38.82 +23:40:46.4: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185738.73+234050.0,2461348.6803,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185738.73+234050.0 20261104.1803 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.37 19:21:09.97 +19:48:39.8
53.87912 2.65000 galactic Vul Second-epoch detections are separated by 1.8" and 7.3 pix
The object was found in VSX 1" ZTF J192109.89+194840.2
Type: SR
# Max. Min./Amp. JD0 Period
13.690 r Y 0.110 r 2458585.64770 225.571542300000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:21:09.97 +19:48:39.8: 14.46 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:21:09.97 +19:48:39.8: 14.34 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192109.89+194840.2,2461348.6803,13.37,0.05,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
ZTF J192109.89+194840.2 20261104.1803 13.37CV 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 11 04.1803 2461348.6803 12.40 19:04:33.28 +24:40:51.8
56.47895 8.28782 galactic Vul Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX 3" ASASSN-V J190433.04+244050.7
Type: SR
# Max. Min./Amp. JD0 Period
13.990 V 14.360 V 2457216.90000 99.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:33.28 +24:40:51.8: 13.76 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:33.28 +24:40:51.8: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190433.04+244050.7,2461348.6803,12.40,0.05,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
ASASSN-V J190433.04+244050.7 20261104.1803 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 11 04.1803 2461348.6803 13.41 19:12:15.22 +21:20:38.1
54.27483 5.20825 galactic Vul Second-epoch detections are separated by 2.0" and 7.0 pix
The object was found in VSX 2" ASASSN-V J191215.08+212038.1
Type: SR
# Max. Min./Amp. JD0 Period
14.550 V 14.650 V 2457959.01000 38.270000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:15.22 +21:20:38.1: 14.50 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:15.22 +21:20:38.1: 14.32 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191215.08+212038.1,2461348.6803,13.41,0.05,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
ASASSN-V J191215.08+212038.1 20261104.1803 13.41CV 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 11 04.1803 2461348.6803 12.49 19:09:13.44 +23:42:57.0
56.08394 6.90506 galactic Vul Second-epoch detections are separated by 0.6" and 7.3 pix
The object was found in VSX 2" ASASSN-V J190913.39+234258.7
Type: SR
# Max. Min./Amp. JD0 Period
14.090 V 14.320 V 2457961.00000 551.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:13.44 +23:42:57.0: 13.65 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:13.44 +23:42:57.0: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190913.39+234258.7,2461348.6803,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190913.39+234258.7 20261104.1803 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.13 19:02:51.26 +25:24:55.2
56.97584 8.95574 galactic Vul Second-epoch detections are separated by 1.8" and 7.4 pix
The object was found in VSX 3" ASASSN-V J190251.12+252457.7
Type: SR
# Max. Min./Amp. JD0 Period
14.210 V 14.540 V 2457204.00000 552.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:02:51.26 +25:24:55.2: 14.07 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:02:51.26 +25:24:55.2: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190251.12+252457.7,2461348.6803,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190251.12+252457.7 20261104.1803 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.48 19:35:36.39 +21:46:10.2
57.21239 0.61930 galactic Vul Second-epoch detections are separated by 3.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:35:36.39 +21:46:10.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:35:36.39 +21:46:10.2: 14.42 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:35:36.39 +21:46:10.2: 14.39 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461348.6803,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261104.1803 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.56 18:50:46.82 +18:29:26.7
49.43747 8.45530 galactic Her Second-epoch detections are separated by 1.0" and 7.7 pix
The object was found in VSX 5" NSVS 11070558
Type: L
# Max. Min./Amp. JD0 Period
11.800 R1 12.250 R1
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:50:46.82 +18:29:26.7: 13.67 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:50:46.82 +18:29:26.7: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 50 46.82 +18 29 26.7 12.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11070558,2461348.6803,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11070558 20261104.1803 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.52 19:14:44.03 +18:56:50.2
52.40688 3.59140 galactic Sge Second-epoch detections are separated by 1.2" and 7.3 pix
The object was found in VSX 2" ASASSN-V J191443.88+185650.6
Type: L
# Max. Min./Amp. JD0 Period
14.200 V 14.460 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:14:44.03 +18:56:50.2: 13.60 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:14:44.03 +18:56:50.2: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191443.88+185650.6,2461348.6803,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191443.88+185650.6 20261104.1803 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.65 19:21:48.73 +23:35:18.9
57.29495 4.28335 galactic Vul Second-epoch detections are separated by 0.5" and 7.1 pix
The object was found in VSX 1" ASASSN-V J192148.75+233519.5
Type: SR
# Max. Min./Amp. JD0 Period
13.890 V 14.120 V 2457238.00000 440.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:21:48.73 +23:35:18.9: 13.61 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:21:48.73 +23:35:18.9: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192148.75+233519.5,2461348.6803,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192148.75+233519.5 20261104.1803 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.26 19:31:34.02 +19:54:00.4
55.11966 0.54018 galactic Vul Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 2" ASASSN-V J193134.13+195402.1
Type: VAR
# Max. Min./Amp. JD0 Period
14.600 V 15.430 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:31:34.02 +19:54:00.4: 14.48 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:31:34.02 +19:54:00.4: 14.58 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193134.13+195402.1,2461348.6803,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193134.13+195402.1 20261104.1803 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.61 19:15:27.13 +23:28:48.0
56.52257 5.52618 galactic Vul Second-epoch detections are separated by 0.6" and 7.3 pix
The object was found in VSX 2" ASASSN-V J191527.09+232849.6
Type: SR
# Max. Min./Amp. JD0 Period
13.910 V 14.040 V 2457677.00000 349.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:15:27.13 +23:28:48.0: 13.57 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:15:27.13 +23:28:48.0: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191527.09+232849.6,2461348.6803,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191527.09+232849.6 20261104.1803 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.46 19:39:21.13 +26:18:43.7
61.59445 2.09430 galactic Vul Second-epoch detections are separated by 0.4" and 7.0 pix
The object was found in VSX 2" ASASSN-V J193921.17+261845.7
Type: SR
# Max. Min./Amp. JD0 Period
14.070 V 14.400 V 2458517.64890 475.873756600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:39:21.13 +26:18:43.7: 13.56 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:39:21.13 +26:18:43.7: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193921.17+261845.7,2461348.6803,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193921.17+261845.7 20261104.1803 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 11 04.1803 2461348.6803 12.59 19:31:50.37 +22:57:36.8
57.83313 1.95764 galactic Vul Second-epoch detections are separated by 2.1" and 7.4 pix
The object was found in VSX 6" ASASSN-V J193150.66+225741.2
Type: SR
# Max. Min./Amp. JD0 Period
14.250 V 14.560 V 2458353.71030 55.134179200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:31:50.37 +22:57:36.8: 13.54 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:31:50.37 +22:57:36.8: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193150.66+225741.2,2461348.6803,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193150.66+225741.2 20261104.1803 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.59 19:01:19.68 +20:28:27.5
52.33914 7.09578 galactic Sge Second-epoch detections are separated by 1.4" and 7.4 pix
The object was found in VSX 3" ASASSN-V J190119.60+202830.1
Type: SR
# Max. Min./Amp. JD0 Period
14.080 V 14.230 V 2458269.87000 39.990000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:01:19.68 +20:28:27.5: 13.56 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:01:19.68 +20:28:27.5: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190119.60+202830.1,2461348.6803,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190119.60+202830.1 20261104.1803 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.66 19:13:34.95 +26:22:44.8
58.92831 7.21988 galactic Lyr Second-epoch detections are separated by 2.0" and 7.3 pix
The object was found in VSX 3" ASASSN-V J191335.15+262243.6
Type: SR
# Max. Min./Amp. JD0 Period
13.170 V 13.610 V 2457311.80000 321.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:13:34.95 +26:22:44.8: 13.55 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:13:34.95 +26:22:44.8: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191335.15+262243.6,2461348.6803,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191335.15+262243.6 20261104.1803 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.44 19:10:34.16 +19:11:06.6
52.16595 4.57482 galactic Sge Second-epoch detections are separated by 1.4" and 7.4 pix
The object was found in VSX 2" ZTF J191034.16+191108.2
Type: SR
# Max. Min./Amp. JD0 Period
13.701 r Y 0.176 r 2458289.03010 26.637510200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:10:34.16 +19:11:06.6: 14.46 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:10:34.16 +19:11:06.6: 14.64 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.54 +/- 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
ZTF J191034.16+191108.2,2461348.6803,13.44,0.05,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
ZTF J191034.16+191108.2 20261104.1803 13.44CV 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 11 04.1803 2461348.6803 12.60 19:09:27.26 +18:49:47.5
51.72813 4.64732 galactic Sge Second-epoch detections are separated by 0.7" and 7.6 pix
The object was found in VSX 4" ZTF J190927.50+184945.7
Type: SR
# Max. Min./Amp. JD0 Period
13.714 r Y 0.204 r 2458541.40880 60.020996600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:27.26 +18:49:47.5: 13.56 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:27.26 +18:49:47.5: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 J190927.50+184945.7,2461348.6803,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190927.50+184945.7 20261104.1803 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.46 19:19:51.09 +21:19:39.1
55.07802 3.63049 galactic Vul Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:19:51.09 +21:19:39.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:19:51.09 +21:19:39.1: 14.46 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:19:51.09 +21:19:39.1: 14.36 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461348.6803,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261104.1803 13.46CV 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 11 04.1803 2461348.6803 12.58 19:20:23.11 +24:24:41.3
57.87396 4.95438 galactic Vul Second-epoch detections are separated by 1.1" and 7.4 pix
The object was found in VSX 4" ASASSN-V J192023.37+242442.9
Type: SR
# Max. Min./Amp. JD0 Period
13.710 V 13.990 V 2458010.85000 48.550000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:20:23.11 +24:24:41.3: 13.49 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:20:23.11 +24:24:41.3: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192023.37+242442.9,2461348.6803,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192023.37+242442.9 20261104.1803 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.40 19:11:21.37 +25:55:53.5
58.29892 7.46536 galactic Lyr Second-epoch detections are separated by 1.3" and 7.4 pix
The object was found in VSX 2" ASASSN-V J191121.31+255554.9
Type: L:
# Max. Min./Amp. JD0 Period
13.930 V 14.600 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:21.37 +25:55:53.5: 13.53 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:21.37 +25:55:53.5: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191121.31+255554.9,2461348.6803,12.40,0.05,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
ASASSN-V J191121.31+255554.9 20261104.1803 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 11 04.1803 2461348.6803 13.34 19:28:32.61 +22:12:07.1
56.80244 2.26245 galactic Vul Second-epoch detections are separated by 0.9" and 7.2 pix
The object was found in VSX 1" ASASSN-V J192832.70+221207.8
Type: SR
# Max. Min./Amp. JD0 Period
15.000 V 15.450 V 2457062.00000 546.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:28:32.61 +22:12:07.1: 14.49 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:28:32.61 +22:12:07.1: 14.50 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.49 +/- 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
ASASSN-V J192832.70+221207.8,2461348.6803,13.34,0.05,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
ASASSN-V J192832.70+221207.8 20261104.1803 13.34CV 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 11 04.1803 2461348.6803 12.53 19:12:41.16 +23:14:43.6
56.02197 5.98439 galactic Vul Second-epoch detections are separated by 1.1" and 7.3 pix
The object was found in VSX 2" ASASSN-V J191241.24+231445.4
Type: L:
# Max. Min./Amp. JD0 Period
13.720 V 14.100 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:41.16 +23:14:43.6: 13.49 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:41.16 +23:14:43.6: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191241.24+231445.4,2461348.6803,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191241.24+231445.4 20261104.1803 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.16 18:58:55.16 +22:29:54.0
53.92381 8.49068 galactic Vul Second-epoch detections are separated by 3.3" and 7.3 pix
The object was found in VSX 3" Mis V0980
Type: M
# Max. Min./Amp. JD0 Period
14.700 V < 18.200 V 2458226.00000 311.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:58:55.16 +22:29:54.0: 14.25 +/- 0.11 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:58:55.16 +22:29:54.0: 14.26 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.25 +/- 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
Mis V0980,2461348.6803,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0980 20261104.1803 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.55 19:10:39.39 +19:03:48.4
52.06675 4.50092 galactic Sge Second-epoch detections are separated by 1.1" and 7.6 pix
The object was found in VSX 0" ASASSN-V J191039.36+190348.5
Type: SR
# Max. Min./Amp. JD0 Period
14.050 V 14.330 V 2457440.00000 608.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:10:39.39 +19:03:48.4: 13.50 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:10:39.39 +19:03:48.4: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191039.36+190348.5,2461348.6803,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191039.36+190348.5 20261104.1803 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.51 19:13:15.22 +19:43:07.2
52.93221 4.25645 galactic Sge Second-epoch detections are separated by 0.4" and 7.3 pix
The object was found in VSX 1" ASASSN-V J191315.31+194307.1
Type: SR
# Max. Min./Amp. JD0 Period
15.180 g Y 0.340 g 2458956.00700
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:13:15.22 +19:43:07.2: 13.50 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:13:15.22 +19:43:07.2: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191315.31+194307.1,2461348.6803,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191315.31+194307.1 20261104.1803 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.38 19:15:05.14 +19:15:09.2
52.71668 3.65858 galactic Sge Second-epoch detections are separated by 2.0" and 7.1 pix
The object was found in VSX 7" ZTF J191505.09+191515.9
Type: SR
# Max. Min./Amp. JD0 Period
16.910 g Y 0.293 g 2458363.93570 44.763916200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:15:05.14 +19:15:09.2: 14.42 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:15:05.14 +19:15:09.2: 14.35 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191505.09+191515.9,2461348.6803,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191505.09+191515.9 20261104.1803 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.98 19:55:25.63 +23:27:13.8
60.96315 -2.49450 galactic Vul Second-epoch detections are separated by 4.5" and 6.6 pix
The object was found in VSX12" ZTF J195526.50+232716.8
Type: SR
# Max. Min./Amp. JD0 Period
16.205 g Y 0.359 g 2458337.01730 49.150554000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:55:25.63 +23:27:13.8: 14.07 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:55:25.63 +23:27:13.8: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195526.50+232716.8,2461348.6803,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195526.50+232716.8 20261104.1803 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.45 19:18:46.36 +16:59:32.5
51.12025 1.83286 galactic Sge Second-epoch detections are separated by 1.3" and 7.2 pix
The object was found in VSX 1" Gaia DR3 4514858836911354752
Type: VAR
# Max. Min./Amp. JD0 Period
12.570 G 12.650 G 0.015540000000 M
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:18:46.36 +16:59:32.5: 14.40 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:18:46.36 +16:59:32.5: 14.40 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4514858836911354752,2461348.6803,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4514858836911354752 20261104.1803 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.35 19:09:43.79 +20:09:13.8
52.94112 5.19194 galactic Sge Second-epoch detections are separated by 3.8" and 7.2 pix
The object was found in VSX 3" ASASSN-V J190943.88+200916.2
Type: SR
# Max. Min./Amp. JD0 Period
14.670 V 14.930 V 2457997.84000 34.330000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:43.79 +20:09:13.8: 14.36 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:43.79 +20:09:13.8: 14.60 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190943.88+200916.2,2461348.6803,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190943.88+200916.2 20261104.1803 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.30 19:02:38.51 +22:49:16.6
54.59799 7.86101 galactic Vul Second-epoch detections are separated by 1.4" and 7.2 pix
The object was found in VSX 1" ASASSN-V J190238.44+224917.6
Type: L:
# Max. Min./Amp. JD0 Period
14.690 V 14.990 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:02:38.51 +22:49:16.6: 14.38 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:02:38.51 +22:49:16.6: 14.44 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190238.44+224917.6,2461348.6803,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190238.44+224917.6 20261104.1803 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.16 19:26:54.27 +23:40:26.7
57.91979 3.29395 galactic Vul Second-epoch detections are separated by 1.1" and 7.0 pix
The object was found in VSX 2" ASASSN-V J192654.29+234028.5
Type: SR
# Max. Min./Amp. JD0 Period
14.580 V 15.360 V 2458335.28230 103.883130200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:26:54.27 +23:40:26.7: 14.32 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:26:54.27 +23:40:26.7: 14.14 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192654.29+234028.5,2461348.6803,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192654.29+234028.5 20261104.1803 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.29 19:15:54.02 +23:41:30.6
56.75901 5.53181 galactic Vul Second-epoch detections are separated by 1.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:15:54.02 +23:41:30.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:15:54.02 +23:41:30.6: 14.38 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:15:54.02 +23:41:30.6: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461348.6803,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261104.1803 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.32 19:44:53.21 +24:17:36.4
60.46104 0.00730 galactic Vul Second-epoch detections are separated by 0.7" and 7.2 pix
The object was found in VSX 1" ASASSN-V J194453.22+241737.4
Type: SR
# Max. Min./Amp. JD0 Period
16.840 g Y 0.700 g 2458738.63500 588.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:44:53.21 +24:17:36.4: 14.35 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:44:53.21 +24:17:36.4: 14.71 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.48 +/- 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
ASASSN-V J194453.22+241737.4,2461348.6803,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194453.22+241737.4 20261104.1803 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.43 19:42:36.43 +25:08:47.5
60.94261 0.88129 galactic Vul Second-epoch detections are separated by 1.1" and 7.1 pix
The object was found in VSX 8" ZTF J194236.82+250853.8
Type: SR
# Max. Min./Amp. JD0 Period
14.293 r Y 0.152 r 2458288.82330 45.297572800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:42:36.43 +25:08:47.5: 14.38 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:42:36.43 +25:08:47.5: 14.46 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194236.82+250853.8,2461348.6803,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194236.82+250853.8 20261104.1803 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.07 19:21:38.56 +25:05:04.8
58.60555 5.01367 galactic Vul Second-epoch detections are separated by 1.1" and 7.3 pix
The object was found in VSX 1" ASASSN-V J192138.52+250503.6
Type: SR
# Max. Min./Amp. JD0 Period
15.000 V 15.310 V 2457079.10000 57.420000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:21:38.56 +25:05:04.8: 14.32 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:21:38.56 +25:05:04.8: 14.23 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192138.52+250503.6,2461348.6803,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192138.52+250503.6 20261104.1803 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.30 18:53:02.65 +23:01:35.7
53.81227 9.94026 galactic Her Second-epoch detections are separated by 0.9" and 7.6 pix
The object was found in VSX 5" NSVS J1853024+230143
Type: SR
# Max. Min./Amp. JD0 Period
15.327 g Y 1.092 g 2458249.68370 191.039995800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:53:02.65 +23:01:35.7: 13.38 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:53:02.65 +23:01:35.7: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 53 02.65 +23 01 35.7 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1853024+230143,2461348.6803,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1853024+230143 20261104.1803 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.11 19:10:20.17 +18:59:47.6
51.97238 4.53774 galactic Sge Second-epoch detections are separated by 6.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:10:20.17 +18:59:47.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:10:20.17 +18:59:47.6: 13.99 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:10:20.17 +18:59:47.6: 14.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461348.6803,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261104.1803 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.30 19:23:06.05 +22:46:36.3
56.71439 3.64199 galactic Vul Second-epoch detections are separated by 1.3" and 7.1 pix
The object was found in VSX 2" ASASSN-V J192306.03+224634.7
Type: SR
# Max. Min./Amp. JD0 Period
14.690 V 14.870 V 2457181.03000 44.240000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:23:06.05 +22:46:36.3: 14.39 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:23:06.05 +22:46:36.3: 14.33 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192306.03+224634.7,2461348.6803,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192306.03+224634.7 20261104.1803 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.35 19:24:43.81 +20:56:00.4
55.26384 2.44090 galactic Vul Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 2" ASASSN-V J192443.71+205602.1
Type: SR
# Max. Min./Amp. JD0 Period
14.920 V 15.130 V 2457989.92000 33.480000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:24:43.81 +20:56:00.4: 14.30 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:24:43.81 +20:56:00.4: 14.34 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.32 +/- 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 J192443.71+205602.1,2461348.6803,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192443.71+205602.1 20261104.1803 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.10 19:04:34.08 +25:57:43.4
57.64434 8.84727 galactic Lyr Second-epoch detections are separated by 0.9" and 7.3 pix
The object was found in VSX10" ZTF J190434.12+255753.4
Type: SR
# Max. Min./Amp. JD0 Period
12.701 r Y 0.254 r 2458266.98900 70.722092200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:34.08 +25:57:43.4: 13.15 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:34.08 +25:57:43.4: 13.25 +/- 0.04 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
ZTF J190434.12+255753.4,2461348.6803,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190434.12+255753.4 20261104.1803 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.34 19:19:56.96 +17:07:46.7
51.37326 1.64855 galactic Sge Second-epoch detections are separated by 2.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:19:56.96 +17:07:46.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:19:56.96 +17:07:46.7: 14.33 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:19:56.96 +17:07:46.7: 14.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461348.6803,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261104.1803 13.34CV 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 11 04.1803 2461348.6803 12.13 19:40:34.48 +23:58:08.3
59.69058 0.69983 galactic Vul Second-epoch detections are separated by 1.7" and 7.1 pix
The object was found in VSX 5" ASASSN-V J194034.62+235812.9
Type: L:
# Max. Min./Amp. JD0 Period
13.960 V 14.300 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:40:34.48 +23:58:08.3: 13.17 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:40:34.48 +23:58:08.3: 13.19 +/- 0.04 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
ASASSN-V J194034.62+235812.9,2461348.6803,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194034.62+235812.9 20261104.1803 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.29 19:40:36.73 +25:02:46.0
60.63173 1.22403 galactic Vul Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX 3" NSVS 8379121
Type: SR
# Max. Min./Amp. JD0 Period
15.061 g Y 0.531 g 2458718.11620 613.398327600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:40:36.73 +25:02:46.0: 13.24 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:40:36.73 +25:02:46.0: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8379121,2461348.6803,12.29,0.05,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
NSVS 8379121 20261104.1803 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 11 04.1803 2461348.6803 13.32 19:31:32.56 +19:49:59.7
55.05830 0.51299 galactic Vul Second-epoch detections are separated by 2.1" and 7.0 pix
The object was found in VSX 4" ZTF J193132.78+195001.7
Type: SR
# Max. Min./Amp. JD0 Period
13.489 r Y 0.110 r 2458644.84530 41.681473600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:31:32.56 +19:49:59.7: 14.22 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:31:32.56 +19:49:59.7: 14.24 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193132.78+195001.7,2461348.6803,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193132.78+195001.7 20261104.1803 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.17 19:11:15.58 +23:01:23.0
55.67317 6.17592 galactic Vul Second-epoch detections are separated by 0.4" and 7.4 pix
The object was found in VSX 1" 2MASS J19111555+2301235
Type: L
# Max. Min./Amp. JD0 Period
11.250 R1 11.630 R1
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:15.58 +23:01:23.0: 13.22 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:15.58 +23:01:23.0: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J19111555+2301235,2461348.6803,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J19111555+2301235 20261104.1803 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.05 19:11:08.80 +20:07:04.0
53.06088 4.87943 galactic Sge Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX 1" ASASSN-V J191108.75+200704.3
Type: SRS
# Max. Min./Amp. JD0 Period
14.660 V 14.920 V 2457209.03000 27.587000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:08.80 +20:07:04.0: 14.28 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:08.80 +20:07:04.0: 14.23 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191108.75+200704.3,2461348.6803,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191108.75+200704.3 20261104.1803 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.24 19:17:36.52 +26:01:42.1
59.02604 6.25594 galactic Lyr Second-epoch detections are separated by 0.5" and 7.2 pix
The object was found in VSX 3" ASASSN-V J191736.60+260145.1
Type: L
# Max. Min./Amp. JD0 Period
13.630 V 13.950 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:17:36.52 +26:01:42.1: 13.21 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:17:36.52 +26:01:42.1: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191736.60+260145.1,2461348.6803,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191736.60+260145.1 20261104.1803 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.31 19:17:29.24 +25:21:17.2
58.41104 5.97217 galactic Vul Second-epoch detections are separated by 1.0" and 7.4 pix
The object was found in VSX 3" ASASSN-V J191729.18+252119.6
Type: SR
# Max. Min./Amp. JD0 Period
13.720 V 13.930 V 2457071.20000 52.410000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:17:29.24 +25:21:17.2: 13.27 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:17:29.24 +25:21:17.2: 13.21 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191729.18+252119.6,2461348.6803,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191729.18+252119.6 20261104.1803 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.96 19:33:34.37 +26:01:17.2
60.70884 3.08596 galactic Vul Second-epoch detections are separated by 1.2" and 6.9 pix
The object was found in VSX 3" NSVS J1933344+260117
Type: SR
# Max. Min./Amp. JD0 Period
16.071 g Y 0.369 g 2458638.05820 117.627882400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:33:34.37 +26:01:17.2: 13.21 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:33:34.37 +26:01:17.2: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1933344+260117,2461348.6803,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1933344+260117 20261104.1803 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.29 19:45:06.35 +18:22:43.0
55.36083 -2.99259 galactic Sge Second-epoch detections are separated by 2.9" and 7.8 pix This object is listed in tocp_transients_list.txt 2.0" PNV J19450648+1822422 2026-08-25.1278 9.0magThe object was found in VSX 2" Gaia DR3 1824166210904571136
Type:
# Max. Min./Amp. JD0 Period
19.340 G 20.790 G 9.901100000000
ATTENTION: measured mag 12.29 is 7.1 mag brighter than the VSX record maximum brightness 19.34 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1824166210904571136,2461348.6803,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1824166210904571136 20261104.1803 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 11 04.1803 2461348.6803 12.07 19:09:27.93 +24:15:29.9
56.59743 7.09888 galactic Vul Second-epoch detections are separated by 4.5" and 7.4 pix
The object was found in VSX 7" ASASSN-V J190928.09+241536.8
Type: SRS
# Max. Min./Amp. JD0 Period
13.390 V 13.530 V 2457945.91000 25.593000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:27.93 +24:15:29.9: 13.14 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:27.93 +24:15:29.9: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190928.09+241536.8,2461348.6803,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190928.09+241536.8 20261104.1803 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.02 19:01:48.83 +21:46:54.5
53.57155 7.57362 galactic Vul Second-epoch detections are separated by 4.2" and 8.1 pix
The object was found in VSX 2" ASASSN-V J190148.83+214652.6
Type: L:
# Max. Min./Amp. JD0 Period
14.550 V 14.850 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:01:48.83 +21:46:54.5: 14.21 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:01:48.83 +21:46:54.5: 14.10 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190148.83+214652.6,2461348.6803,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190148.83+214652.6 20261104.1803 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.35 19:09:13.19 +22:04:03.1
54.60173 6.16448 galactic Vul Second-epoch detections are separated by 1.1" and 7.5 pix
The object was found in VSX 2" ASASSN-V J190913.14+220404.5
Type: SR
# Max. Min./Amp. JD0 Period
14.730 V 15.010 V 2457825.09000 32.850000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:13.19 +22:04:03.1: 14.25 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:13.19 +22:04:03.1: 14.45 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.33 +/- 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 J190913.14+220404.5,2461348.6803,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190913.14+220404.5 20261104.1803 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.12 19:04:37.40 +22:16:09.2
54.30327 7.20625 galactic Vul Second-epoch detections are separated by 1.0" and 7.6 pix
The object was found in VSX 1" ASAS J190438+2216.2
Type: MISC
# Max. Min./Amp. JD0 Period
12.867 V Y 1.277 V 128.891071000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:37.40 +22:16:09.2: 13.16 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:37.40 +22:16:09.2: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190438+2216.2,2461348.6803,12.12,0.05,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
ASAS J190438+2216.2 20261104.1803 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 11 04.1803 2461348.6803 12.82 19:06:18.03 +23:50:04.4
55.89008 7.55657 galactic Vul Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX 2" Dauban V79
Type: SR
# Max. Min./Amp. JD0 Period
13.210 r Y 0.668 r 2458322.54810 144.300320400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:06:18.03 +23:50:04.4: 14.21 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:06:18.03 +23:50:04.4: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Dauban V79,2461348.6803,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Dauban V79 20261104.1803 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.16 19:37:10.15 +18:11:20.3
54.26542 -1.44750 galactic Sge Second-epoch detections are separated by 0.7" and 7.4 pix
The object was found in VSX 1" ZTF J193710.13+181119.7
Type: SR
# Max. Min./Amp. JD0 Period
14.840 g Y 0.215 g 2458383.88310 48.162798900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:10.15 +18:11:20.3: 13.12 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:10.15 +18:11:20.3: 13.16 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193710.13+181119.7,2461348.6803,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193710.13+181119.7 20261104.1803 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.32 19:36:46.07 +25:24:56.3
60.52742 2.16292 galactic Vul Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX 4" ZTF J193646.16+252459.6
Type: SR
# Max. Min./Amp. JD0 Period
16.376 g Y 0.307 g 2458330.80830 47.391948100000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:36:46.07 +25:24:56.3: 14.18 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:36:46.07 +25:24:56.3: 14.28 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193646.16+252459.6,2461348.6803,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193646.16+252459.6 20261104.1803 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.93 18:55:25.62 +22:25:43.9
53.50526 9.18693 galactic Her Second-epoch detections are separated by 1.2" and 7.7 pix
The object was found in VSX 7" ASASSN-V J185525.13+222542.4
Type: L:
# Max. Min./Amp. JD0 Period
13.770 V 14.120 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:55:25.62 +22:25:43.9: 13.04 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:55:25.62 +22:25:43.9: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 55 25.62 +22 25 43.9 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185525.13+222542.4,2461348.6803,11.93,0.05,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
ASASSN-V J185525.13+222542.4 20261104.1803 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 11 04.1803 2461348.6803 13.28 19:16:58.11 +17:56:55.6
51.76644 2.65925 galactic Sge Second-epoch detections are separated by 3.1" and 7.1 pix
The object was found in VSX 1" ASASSN-V J191658.06+175656.2
Type: SRS
# Max. Min./Amp. JD0 Period
15.110 V 15.260 V 2457209.03000 11.702000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:16:58.11 +17:56:55.6: 14.20 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:16:58.11 +17:56:55.6: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191658.06+175656.2,2461348.6803,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191658.06+175656.2 20261104.1803 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.14 18:51:56.48 +21:48:11.3
52.57995 9.64516 galactic Her Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 3" ASASSN-V J185156.27+214811.7
Type: L
# Max. Min./Amp. JD0 Period
13.570 V 14.100 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:51:56.48 +21:48:11.3: 13.10 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:51:56.48 +21:48:11.3: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 51 56.48 +21 48 11.3 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185156.27+214811.7,2461348.6803,12.14,0.05,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
ASASSN-V J185156.27+214811.7 20261104.1803 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 11 04.1803 2461348.6803 13.03 19:38:20.76 +24:43:00.1
60.09202 1.50957 galactic Vul Second-epoch detections are separated by 3.2" and 7.1 pix
The object was found in VSX 2" ZTF J193820.72+244301.8
Type: SR
# Max. Min./Amp. JD0 Period
13.581 r Y 0.591 r 2458260.99710 147.892854800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:20.76 +24:43:00.1: 14.19 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:20.76 +24:43:00.1: 14.17 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193820.72+244301.8,2461348.6803,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193820.72+244301.8 20261104.1803 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.19 19:01:04.19 +25:18:27.2
56.69994 9.27184 galactic Vul Second-epoch detections are separated by 0.7" and 7.5 pix
The object was found in VSX 2" ZTF J190104.04+251827.8
Type: SR
# Max. Min./Amp. JD0 Period
12.514 r Y 0.226 r 2458370.98950 59.730878200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:01:04.19 +25:18:27.2: 13.11 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:01:04.19 +25:18:27.2: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190104.04+251827.8,2461348.6803,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190104.04+251827.8 20261104.1803 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.15 19:13:06.67 +20:14:10.4
53.37805 4.52360 galactic Sge Second-epoch detections are separated by 1.5" and 7.5 pix
The object was found in VSX 1" ASASSN-V J191306.68+201411.4
Type: SR
# Max. Min./Amp. JD0 Period
15.620 g Y 0.480 g 2458729.48400 208.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:13:06.67 +20:14:10.4: 14.17 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:13:06.67 +20:14:10.4: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191306.68+201411.4,2461348.6803,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191306.68+201411.4 20261104.1803 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.19 19:31:30.63 +26:07:04.2
60.57078 3.53849 galactic Vul Second-epoch detections are separated by 4.2" and 6.9 pix
The object was found in VSX 4" ASASSN-V J193130.91+260703.2
Type: SR
# Max. Min./Amp. JD0 Period
14.610 V 14.840 V 2457512.03000 31.770000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:31:30.63 +26:07:04.2: 14.12 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:31:30.63 +26:07:04.2: 14.12 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193130.91+260703.2,2461348.6803,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193130.91+260703.2 20261104.1803 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.24 19:10:28.53 +25:43:55.9
58.02971 7.55348 galactic Lyr Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX 2" ASASSN-V J191028.51+254358.3
Type: SR
# Max. Min./Amp. JD0 Period
14.050 V 14.800 V 2457069.20000 63.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:10:28.53 +25:43:55.9: 14.19 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:10:28.53 +25:43:55.9: 14.14 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 J191028.51+254358.3,2461348.6803,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191028.51+254358.3 20261104.1803 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.96 18:50:46.51 +20:52:25.8
51.61080 9.49009 galactic Her Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX 9" ASASSN-V J185045.89+205227.5
Type: SR
# Max. Min./Amp. JD0 Period
15.720 g Y 0.660 g 2458754.57900 298.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:50:46.51 +20:52:25.8: 14.17 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:50:46.51 +20:52:25.8: 14.12 +/- 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!
TCP 2026 11 04.1803* 18 50 46.51 +20 52 25.8 13.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185045.89+205227.5,2461348.6803,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185045.89+205227.5 20261104.1803 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.17 19:12:46.73 +19:31:41.7
52.71110 4.26842 galactic Sge Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX 1" V0385 Sge
Type: SR
# Max. Min./Amp. JD0 Period
14.100 R Y 0.060 R 39.000000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:46.73 +19:31:41.7: 14.18 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:46.73 +19:31:41.7: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0385 Sge,2461348.6803,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0385 Sge 20261104.1803 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.34 19:26:27.15 +21:54:37.6
56.31521 2.55010 galactic Vul Second-epoch detections are separated by 2.5" and 6.8 pix
The object was found in VSX 4" NSVS J1926270+215440
Type: M
# Max. Min./Amp. JD0 Period
15.549 r Y 3.430 r 2458363.91360 309.782929100000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:26:27.15 +21:54:37.6: 15.01 +/- 0.15 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:26:27.15 +21:54:37.6: 14.78 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.88 +/- 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
NSVS J1926270+215440,2461348.6803,13.34,0.05,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
NSVS J1926270+215440 20261104.1803 13.34CV 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 11 04.1803 2461348.6803 12.14 19:10:45.25 +24:37:51.3
57.06554 7.00384 galactic Vul Second-epoch detections are separated by 0.8" and 7.3 pix
The object was found in VSX 2" ASASSN-V J191045.12+243752.2
Type: SR
# Max. Min./Amp. JD0 Period
14.470 g Y 0.440 g 2459385.83500 31.450000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:10:45.25 +24:37:51.3: 13.04 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:10:45.25 +24:37:51.3: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191045.12+243752.2,2461348.6803,12.14,0.05,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
ASASSN-V J191045.12+243752.2 20261104.1803 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 11 04.1803 2461348.6803 12.08 19:00:04.96 +21:11:47.5
52.86231 7.67638 galactic Sge Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX 2" ASASSN-V J190004.83+211148.0
Type: SR
# Max. Min./Amp. JD0 Period
13.740 V 14.200 V 2458347.23990 166.335373900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:00:04.96 +21:11:47.5: 13.01 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:00:04.96 +21:11:47.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190004.83+211148.0,2461348.6803,12.08,0.05,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
ASASSN-V J190004.83+211148.0 20261104.1803 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 11 04.1803 2461348.6803 13.15 19:11:10.27 +19:26:32.1
52.46044 4.56591 galactic Sge Second-epoch detections are separated by 2.2" and 7.7 pix
The object was found in VSX 1" ASASSN-V J191110.23+192632.8
Type: SR
# Max. Min./Amp. JD0 Period
15.580 g Y 0.540 g 2459534.56500 579.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:10.27 +19:26:32.1: 14.22 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:10.27 +19:26:32.1: 14.15 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.19 +/- 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 J191110.23+192632.8,2461348.6803,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191110.23+192632.8 20261104.1803 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.21 19:13:27.45 +19:56:12.9
53.14871 4.31405 galactic Sge Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:13:27.45 +19:56:12.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:13:27.45 +19:56:12.9: 14.22 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:13:27.45 +19:56:12.9: 14.43 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461348.6803,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261104.1803 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.86 19:11:28.80 +25:39:16.6
58.06187 7.31638 galactic Vul Second-epoch detections are separated by 0.5" and 7.2 pix
The object was found in VSX 2" ASAS J191129+2539.3
Type: MISC
# Max. Min./Amp. JD0 Period
12.930 V Y 0.877 V 0.999860000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:28.80 +25:39:16.6: 13.00 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:28.80 +25:39:16.6: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J191129+2539.3,2461348.6803,11.86,0.05,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
ASAS J191129+2539.3 20261104.1803 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 11 04.1803 2461348.6803 13.13 19:14:56.57 +24:59:41.7
57.82482 6.32034 galactic Vul Second-epoch detections are separated by 0.8" and 7.4 pix
The object was found in VSX 2" ASASSN-V J191456.43+245942.5
Type: SR
# Max. Min./Amp. JD0 Period
15.920 g Y 0.860 g 2458700.80700 598.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:14:56.57 +24:59:41.7: 14.20 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:14:56.57 +24:59:41.7: 14.17 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191456.43+245942.5,2461348.6803,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191456.43+245942.5 20261104.1803 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.14 19:17:19.37 +18:22:16.5
52.18009 2.78111 galactic Sge Second-epoch detections are separated by 1.8" and 7.2 pix
The object was found in VSX 5" ZTF J191719.64+182213.6
Type: SR
# Max. Min./Amp. JD0 Period
13.682 r Y 0.102 r 2458329.44430 140.311621700000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:17:19.37 +18:22:16.5: 14.21 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:17:19.37 +18:22:16.5: 14.36 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191719.64+182213.6,2461348.6803,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191719.64+182213.6 20261104.1803 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.93 19:05:23.82 +19:44:23.9
52.10772 5.91305 galactic Sge Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX 1" ASASSN-V J190523.83+194425.0
Type: SR
# Max. Min./Amp. JD0 Period
13.340 V 13.800 V 2458303.79960 49.288160000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:05:23.82 +19:44:23.9: 12.97 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:05:23.82 +19:44:23.9: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190523.83+194425.0,2461348.6803,11.93,0.05,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
ASASSN-V J190523.83+194425.0 20261104.1803 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 11 04.1803 2461348.6803 12.05 19:24:05.81 +26:32:44.3
60.16190 5.20463 galactic Vul Second-epoch detections are separated by 0.6" and 7.1 pix
The object was found in VSX 2" ASAS J192406+2632.7
Type: MISC
# Max. Min./Amp. JD0 Period
12.584 V Y 0.953 V 105.022354000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:24:05.81 +26:32:44.3: 12.99 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:24:05.81 +26:32:44.3: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J192406+2632.7,2461348.6803,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J192406+2632.7 20261104.1803 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.25 19:12:14.83 +20:15:55.0
53.31090 4.71707 galactic Sge Second-epoch detections are separated by 3.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:12:14.83 +20:15:55.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:14.83 +20:15:55.0: 14.18 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:14.83 +20:15:55.0: 14.36 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461348.6803,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261104.1803 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.19 19:22:55.04 +24:09:57.5
57.92528 4.32940 galactic Vul Second-epoch detections are separated by 1.6" and 7.5 pix
The object was found in VSX 1" ASASSN-V J192255.09+240958.4
Type: SR
# Max. Min./Amp. JD0 Period
15.420 g Y 0.680 g 2459408.63500 71.260000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:22:55.04 +24:09:57.5: 14.13 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:22:55.04 +24:09:57.5: 14.05 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 J192255.09+240958.4,2461348.6803,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192255.09+240958.4 20261104.1803 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.05 19:16:11.78 +25:02:27.7
57.99620 6.08852 galactic Vul Second-epoch detections are separated by 0.8" and 7.2 pix
The object was found in VSX 2" ASASSN-V J191611.69+250228.9
Type: L:
# Max. Min./Amp. JD0 Period
13.000 V 13.400 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:16:11.78 +25:02:27.7: 12.93 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:16:11.78 +25:02:27.7: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191611.69+250228.9,2461348.6803,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191611.69+250228.9 20261104.1803 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.20 19:09:14.98 +19:23:11.5
52.20344 4.94377 galactic Sge Second-epoch detections are separated by 1.1" and 7.3 pix
The object was found in VSX 3" ZTF J190915.04+192313.9
Type: SR
# Max. Min./Amp. JD0 Period
16.031 g Y 0.098 g 2458306.88390 23.168437100000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:14.98 +19:23:11.5: 14.17 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:14.98 +19:23:11.5: 14.20 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190915.04+192313.9,2461348.6803,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190915.04+192313.9 20261104.1803 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.20 19:25:28.98 +24:17:10.1
58.30675 3.86918 galactic Vul Second-epoch detections are separated by 0.8" and 7.1 pix
The object was found in VSX 1" ASASSN-V J192528.96+241711.4
Type: SR
# Max. Min./Amp. JD0 Period
15.660 g Y 0.620 g 2458763.56300 381.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:25:28.98 +24:17:10.1: 14.11 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:25:28.98 +24:17:10.1: 14.21 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 J192528.96+241711.4,2461348.6803,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192528.96+241711.4 20261104.1803 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.08 19:42:53.52 +25:50:57.5
61.58459 1.17458 galactic Vul Second-epoch detections are separated by 1.8" and 7.3 pix
The object was found in VSX 3" ZTF J194253.72+255058.9
Type: SR
# Max. Min./Amp. JD0 Period
13.748 r Y 0.437 r 2458471.15100 541.180950000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:42:53.52 +25:50:57.5: 14.18 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:42:53.52 +25:50:57.5: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194253.72+255058.9,2461348.6803,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194253.72+255058.9 20261104.1803 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.24 19:43:53.74 +21:01:40.8
57.51732 -1.42506 galactic Vul Second-epoch detections are separated by 2.8" and 7.7 pix
The object was found in VSX 3" ZTF J194353.88+210138.6
Type: SR
# Max. Min./Amp. JD0 Period
16.903 g Y 0.379 g 2458607.18460 61.930402600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:43:53.74 +21:01:40.8: 14.20 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:43:53.74 +21:01:40.8: 14.30 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194353.88+210138.6,2461348.6803,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194353.88+210138.6 20261104.1803 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.99 19:07:08.11 +18:59:17.0
51.61951 5.20783 galactic Sge Second-epoch detections are separated by 1.6" and 7.5 pix
The object was found in VSX 1" NSVS 11198030
Type: L
# Max. Min./Amp. JD0 Period
10.700 R1 11.300 R1
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:07:08.11 +18:59:17.0: 12.89 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:07:08.11 +18:59:17.0: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11198030,2461348.6803,11.99,0.05,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
NSVS 11198030 20261104.1803 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 11 04.1803 2461348.6803 12.90 18:59:33.41 +25:19:57.2
56.57279 9.59089 galactic Vul Second-epoch detections are separated by 0.9" and 7.3 pix
The object was found in VSX 1" ASASSN-V J185933.33+251956.7
Type: SR
# Max. Min./Amp. JD0 Period
15.290 g Y 0.310 g 2458745.84200 202.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:59:33.41 +25:19:57.2: 14.12 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:59:33.41 +25:19:57.2: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 J185933.33+251956.7,2461348.6803,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185933.33+251956.7 20261104.1803 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.10 19:11:16.89 +17:51:52.5
51.06602 3.82044 galactic Sge Second-epoch detections are separated by 1.8" and 7.8 pix
The object was found in VSX 2" KK Sge
Type: M
# Max. Min./Amp. JD0 Period
6.300 I 12.100 I 2441660.00000 429.300000000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:16.89 +17:51:52.5: 14.16 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:16.89 +17:51:52.5: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.16 +/- 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
KK Sge,2461348.6803,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KK Sge 20261104.1803 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.94 19:41:49.63 +26:10:38.7
61.75091 1.54505 galactic Vul Second-epoch detections are separated by 0.5" and 7.1 pix
The object was found in VSX 6" NSVS J1941500+261042
Type: L:
# Max. Min./Amp. JD0 Period
10.919 R1 Y 0.337 R1 171.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:49.63 +26:10:38.7: 12.87 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:49.63 +26:10:38.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1941500+261042,2461348.6803,11.94,0.05,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
NSVS J1941500+261042 20261104.1803 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 11 04.1803 2461348.6803 11.99 19:09:06.61 +24:55:01.5
57.15509 7.46564 galactic Vul Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 2" NSVS J1909066+245503
Type: L:
# Max. Min./Amp. JD0 Period
11.248 R1 Y 0.374 R1 69.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:06.61 +24:55:01.5: 12.88 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:06.61 +24:55:01.5: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1909066+245503,2461348.6803,11.99,0.05,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
NSVS J1909066+245503 20261104.1803 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 11 04.1803 2461348.6803 11.91 19:17:02.90 +21:30:04.1
54.92887 4.28901 galactic Vul Second-epoch detections are separated by 1.0" and 7.2 pix
The object was found in VSX 1" ASASSN-V J191702.87+213003.3
Type: SR
# Max. Min./Amp. JD0 Period
13.180 V 13.880 V 2457201.90000 89.900000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:17:02.90 +21:30:04.1: 12.86 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:17:02.90 +21:30:04.1: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191702.87+213003.3,2461348.6803,11.91,0.05,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
ASASSN-V J191702.87+213003.3 20261104.1803 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 11 04.1803 2461348.6803 13.13 19:31:55.92 +26:11:20.9
60.67888 3.48959 galactic Vul Second-epoch detections are separated by 3.2" and 6.9 pix
The object was found in VSX 2" ASASSN-V J193155.81+261121.6
Type: SR
# Max. Min./Amp. JD0 Period
15.910 g Y 0.570 g 2458398.54500 333.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:31:55.92 +26:11:20.9: 14.18 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:31:55.92 +26:11:20.9: 14.22 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.20 +/- 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
ASASSN-V J193155.81+261121.6,2461348.6803,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193155.81+261121.6 20261104.1803 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.10 19:20:26.46 +25:52:12.4
59.17868 5.61768 galactic Lyr Second-epoch detections are separated by 1.3" and 6.9 pix
The object was found in VSX 3" ASASSN-V J192026.49+255215.0
Type: SR
# Max. Min./Amp. JD0 Period
14.260 V 14.460 V 2457523.96000 48.550000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:20:26.46 +25:52:12.4: 14.14 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:20:26.46 +25:52:12.4: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192026.49+255215.0,2461348.6803,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192026.49+255215.0 20261104.1803 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.87 19:10:00.84 +24:22:08.4
56.75357 7.03678 galactic Vul Second-epoch detections are separated by 0.4" and 7.3 pix
The object was found in VSX 2" ASASSN-V J191000.80+242210.3
Type: SR
# Max. Min./Amp. JD0 Period
13.200 V 13.430 V 2457223.00000 660.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:10:00.84 +24:22:08.4: 12.85 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:10:00.84 +24:22:08.4: 12.80 +/- 0.02 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
ASASSN-V J191000.80+242210.3,2461348.6803,11.87,0.05,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
ASASSN-V J191000.80+242210.3 20261104.1803 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 11 04.1803 2461348.6803 12.91 19:21:45.26 +24:11:49.1
57.82871 4.57849 galactic Vul Second-epoch detections are separated by 1.9" and 7.6 pix
The object was found in VSX 3" Gaia DR3 2022967838804818944
Type: SR|M
# Max. Min./Amp. JD0 Period
11.370 G 11.870 G 73.720000000000 M
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:21:45.26 +24:11:49.1: 14.14 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:21:45.26 +24:11:49.1: 14.18 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2022967838804818944,2461348.6803,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2022967838804818944 20261104.1803 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.93 19:16:02.54 +24:59:07.1
57.93033 6.09415 galactic Vul Second-epoch detections are separated by 4.5" and 7.1 pix
The object was found in VSX 3" ASASSN-V J191602.38+245904.3
Type: SR
# Max. Min./Amp. JD0 Period
15.270 g Y 0.480 g 2458722.53500 572.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:16:02.54 +24:59:07.1: 14.13 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:16:02.54 +24:59:07.1: 14.07 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191602.38+245904.3,2461348.6803,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191602.38+245904.3 20261104.1803 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.82 19:14:01.25 +22:32:19.9
55.53046 5.38894 galactic Vul Second-epoch detections are separated by 0.6" and 7.4 pix
The object was found in VSX 1" ASASSN-V J191401.16+223220.7
Type: SR
# Max. Min./Amp. JD0 Period
13.240 V 13.580 V 2458255.91420 48.129318400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:14:01.25 +22:32:19.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:14:01.25 +22:32:19.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191401.16+223220.7,2461348.6803,11.82,0.05,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
ASASSN-V J191401.16+223220.7 20261104.1803 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 11 04.1803 2461348.6803 13.03 19:34:11.94 +19:58:28.2
55.48371 0.03458 galactic Vul Second-epoch detections are separated by 1.0" and 7.4 pix
The object was found in VSX 6" NSVS J1934118+195833
Type: M
# Max. Min./Amp. JD0 Period
15.882 r Y 4.588 r 2458498.19690 427.024775200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:34:11.94 +19:58:28.2: 14.03 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:34:11.94 +19:58:28.2: 14.19 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1934118+195833,2461348.6803,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1934118+195833 20261104.1803 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.72 19:20:35.75 +26:05:56.7
59.39894 5.69247 galactic Lyr Second-epoch detections are separated by 0.8" and 7.1 pix
The object was found in VSX 2" ASAS J192036+2606.0
Type: SR
# Max. Min./Amp. JD0 Period
13.000 V 14.000 V 2453484.00000 487.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:20:35.75 +26:05:56.7: 12.74 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:20:35.75 +26:05:56.7: 12.76 +/- 0.02 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
ASAS J192036+2606.0,2461348.6803,11.72,0.05,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
ASAS J192036+2606.0 20261104.1803 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 11 04.1803 2461348.6803 13.68 19:20:10.97 +21:17:23.2
55.08058 3.54462 galactic Sge Second-epoch detections are separated by 2.5" and 7.7 pix
The object was found in VSX 0" ZTF J192010.96+211723.3
Type: SR
# Max. Min./Amp. JD0 Period
14.014 r Y 0.565 r 2458560.23450 453.984159500000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:20:10.97 +21:17:23.2: 14.92 +/- 0.13 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:20:10.97 +21:17:23.2: 14.65 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.75 +/- 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
ZTF J192010.96+211723.3,2461348.6803,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192010.96+211723.3 20261104.1803 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.90 19:20:55.77 +18:47:27.5
52.95100 2.22124 galactic Sge Second-epoch detections are separated by 1.1" and 7.4 pix
The object was found in VSX 2" ZTF J192055.89+184728.7
Type: SR
# Max. Min./Amp. JD0 Period
13.785 r Y 0.194 r 2458647.75370 49.445321200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:20:55.77 +18:47:27.5: 14.02 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:20:55.77 +18:47:27.5: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192055.89+184728.7,2461348.6803,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192055.89+184728.7 20261104.1803 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.64 19:12:10.30 +24:18:34.4
56.92287 6.57114 galactic Vul Second-epoch detections are separated by 0.8" and 7.3 pix
The object was found in VSX 2" ASASSN-V J191210.25+241836.0
Type: SR
# Max. Min./Amp. JD0 Period
12.960 V 13.160 V 2458316.00000 339.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:10.30 +24:18:34.4: 12.71 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:10.30 +24:18:34.4: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191210.25+241836.0,2461348.6803,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191210.25+241836.0 20261104.1803 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.71 19:13:41.77 +26:37:44.3
59.16478 7.30963 galactic Lyr Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 2" HH Lyr
Type: L
# Max. Min./Amp. JD0 Period
14.100 pg 15.200 pg
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:13:41.77 +26:37:44.3: 12.69 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:13:41.77 +26:37:44.3: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HH Lyr,2461348.6803,11.71,0.05,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
HH Lyr 20261104.1803 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 11 04.1803 2461348.6803 13.48 19:04:31.95 +26:09:09.7
57.81434 8.93780 galactic Lyr Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX 4" ASASSN-V J190431.75+260912.3
Type: SR
# Max. Min./Amp. JD0 Period
14.660 V 15.110 V 2457166.90000 72.900000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:31.95 +26:09:09.7: 14.88 +/- 0.17 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:31.95 +26:09:09.7: 14.85 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190431.75+260912.3,2461348.6803,13.48,0.05,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
ASASSN-V J190431.75+260912.3 20261104.1803 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.04 19:17:52.50 +19:05:42.0
52.88252 3.00190 galactic Sge Second-epoch detections are separated by 1.5" and 7.6 pix
The object was found in VSX 4" Gaia DR3 4515405534709557632
Type: L
# Max. Min./Amp. JD0 Period
17.910 G 18.130 G
ATTENTION: measured mag 13.04 is 4.9 mag brighter than the VSX record maximum brightness 17.91 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:17:52.50 +19:05:42.0: 14.05 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:17:52.50 +19:05:42.0: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4515405534709557632,2461348.6803,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4515405534709557632 20261104.1803 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.22 19:23:04.43 +18:35:57.1
53.02051 1.68290 galactic Sge Second-epoch detections are separated by 2.1" and 7.6 pix
The object was found in VSX 2" ZTF J192304.54+183556.9
Type: SR
# Max. Min./Amp. JD0 Period
13.517 r Y 0.153 r 2458276.17380 133.803549000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:23:04.43 +18:35:57.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:23:04.43 +18:35:57.1: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192304.54+183556.9,2461348.6803,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192304.54+183556.9 20261104.1803 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.65 19:14:41.04 +19:15:01.6
52.67097 3.74171 galactic Sge Second-epoch detections are separated by 3.3" and 7.8 pix
The object was found in VSX 9" ZTF J191441.69+191500.2
Type: SR
# Max. Min./Amp. JD0 Period
13.146 r Y 0.192 r 2458643.83740 49.198722600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:14:41.04 +19:15:01.6: 13.63 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:14:41.04 +19:15:01.6: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191441.69+191500.2,2461348.6803,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191441.69+191500.2 20261104.1803 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.92 19:35:19.57 +17:24:41.7
53.37252 -1.44311 galactic Sge Second-epoch detections are separated by 0.5" and 7.4 pix
The object was found in VSX 2" ASASSN-V J193519.56+172439.5
Type: SR
# Max. Min./Amp. JD0 Period
14.300 V 15.500 V 2457217.90000 198.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:35:19.57 +17:24:41.7: 14.11 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:35:19.57 +17:24:41.7: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193519.56+172439.5,2461348.6803,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193519.56+172439.5 20261104.1803 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.09 18:57:41.63 +23:24:27.7
54.62792 9.14060 galactic Vul Second-epoch detections are separated by 1.6" and 7.4 pix
The object was found in VSX 3" ASASSN-V J185741.45+232429.7
Type: SR
# Max. Min./Amp. JD0 Period
14.860 g Y 0.450 g 2459366.08800 298.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:57:41.63 +23:24:27.7: 14.10 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:57:41.63 +23:24:27.7: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185741.45+232429.7,2461348.6803,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185741.45+232429.7 20261104.1803 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.60 19:07:08.69 +25:24:15.4
57.39617 8.08052 galactic Vul Second-epoch detections are separated by 0.6" and 7.4 pix
The object was found in VSX 1" ASASSN-V J190708.73+252415.8
Type: L:
# Max. Min./Amp. JD0 Period
12.890 V 13.380 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:07:08.69 +25:24:15.4: 12.64 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:07:08.69 +25:24:15.4: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190708.73+252415.8,2461348.6803,11.60,0.05,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
ASASSN-V J190708.73+252415.8 20261104.1803 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 11 04.1803 2461348.6803 13.15 19:08:01.85 +24:09:34.7
56.36107 7.34740 galactic Vul Second-epoch detections are separated by 0.9" and 7.2 pix
The object was found in VSX 3" ASASSN-V J190801.79+240937.1
Type: SR
# Max. Min./Amp. JD0 Period
15.480 g Y 0.510 g 2459059.76500 46.290000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:08:01.85 +24:09:34.7: 14.03 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:08:01.85 +24:09:34.7: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190801.79+240937.1,2461348.6803,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190801.79+240937.1 20261104.1803 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.04 19:10:15.92 +18:48:39.0
51.79896 4.46786 galactic Sge Second-epoch detections are separated by 0.8" and 7.4 pix
The object was found in VSX 1" ASASSN-V J191015.97+184838.8
Type: SR
# Max. Min./Amp. JD0 Period
14.250 V 14.480 V 2457333.70000 47.810000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:10:15.92 +18:48:39.0: 14.03 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:10:15.92 +18:48:39.0: 14.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191015.97+184838.8,2461348.6803,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191015.97+184838.8 20261104.1803 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.90 19:13:46.16 +23:09:28.1
56.05731 5.72283 galactic Vul Second-epoch detections are separated by 1.3" and 7.1 pix
The object was found in VSX 2" ASASSN-V J191346.32+230928.5
Type: SR
# Max. Min./Amp. JD0 Period
14.700 V 14.900 V 2457985.00000 592.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:13:46.16 +23:09:28.1: 13.94 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:13:46.16 +23:09:28.1: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191346.32+230928.5,2461348.6803,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191346.32+230928.5 20261104.1803 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.88 19:04:12.03 +25:17:58.8
57.00515 8.63166 galactic Vul Second-epoch detections are separated by 2.8" and 7.6 pix
The object was found in VSX 8" ASASSN-V J190412.64+251759.4
Type: SR
# Max. Min./Amp. JD0 Period
14.010 V 14.850 V 2457084.10000 224.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:12.03 +25:17:58.8: 13.94 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:12.03 +25:17:58.8: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190412.64+251759.4,2461348.6803,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190412.64+251759.4 20261104.1803 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.05 19:04:13.03 +23:58:52.3
55.81004 8.04843 galactic Vul Second-epoch detections are separated by 1.7" and 7.6 pix
The object was found in VSX 1" ASASSN-V J190413.03+235853.7
Type: SR
# Max. Min./Amp. JD0 Period
14.090 V 14.480 V 2457221.90000 52.700000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:13.03 +23:58:52.3: 13.99 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:13.03 +23:58:52.3: 14.09 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190413.03+235853.7,2461348.6803,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190413.03+235853.7 20261104.1803 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.06 19:31:02.92 +24:48:43.5
59.37247 3.00502 galactic Vul Second-epoch detections are separated by 2.9" and 7.5 pix
The object was found in VSX 0" ASASSN-V J193102.91+244843.3
Type: SR
# Max. Min./Amp. JD0 Period
15.200 V 15.800 V 2457533.00000 167.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:31:02.92 +24:48:43.5: 14.01 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:31:02.92 +24:48:43.5: 14.25 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193102.91+244843.3,2461348.6803,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193102.91+244843.3 20261104.1803 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.31 18:56:24.44 +22:00:30.1
53.22142 8.80002 galactic Her Second-epoch detections are separated by 0.4" and 7.4 pix
The object was found in VSX 3" ASAS J185624+2200.5
Type: MISC
# Max. Min./Amp. JD0 Period
9.063 Ic Y 0.203 Ic 2452551.10000 75.070000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:56:24.44 +22:00:30.1: 12.36 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:56:24.44 +22:00:30.1: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 56 24.44 +22 00 30.1 11.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185624+2200.5,2461348.6803,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J185624+2200.5 20261104.1803 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.91 19:24:49.77 +21:56:45.4
56.16831 2.89853 galactic Vul Second-epoch detections are separated by 0.7" and 7.2 pix
The object was found in VSX 2" ASASSN-V J192449.91+215646.0
Type: SR
# Max. Min./Amp. JD0 Period
14.380 V 14.900 V 2458283.90670 213.021733800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:24:49.77 +21:56:45.4: 14.01 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:24:49.77 +21:56:45.4: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192449.91+215646.0,2461348.6803,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192449.91+215646.0 20261104.1803 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.98 19:30:31.21 +24:53:03.7
59.37860 3.14488 galactic Vul Second-epoch detections are separated by 1.7" and 7.3 pix
The object was found in VSX 2" ZTF J193031.20+245305.3
Type: SR
# Max. Min./Amp. JD0 Period
15.506 g Y 0.437 g 2458619.08920 217.229706900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:30:31.21 +24:53:03.7: 13.98 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:30:31.21 +24:53:03.7: 14.01 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193031.20+245305.3,2461348.6803,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193031.20+245305.3 20261104.1803 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.43 19:00:55.84 +24:14:59.4
55.72158 8.84019 galactic Vul Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 2" ASAS J190056+2415.0
Type: MISC
# Max. Min./Amp. JD0 Period
9.119 Ic Y 0.151 Ic 2452526.30000 53.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:00:55.84 +24:14:59.4: 12.32 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:00:55.84 +24:14:59.4: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190056+2415.0,2461348.6803,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190056+2415.0 20261104.1803 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.73 19:02:35.08 +19:11:56.7
51.32248 6.26277 galactic Sge Second-epoch detections are separated by 1.0" and 7.4 pix
The object was found in VSX 4" Gaia DR3 4517794734810380800
Type: L
# Max. Min./Amp. JD0 Period
12.040 G 12.330 G M
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:02:35.08 +19:11:56.7: 13.78 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:02:35.08 +19:11:56.7: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 4517794734810380800,2461348.6803,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4517794734810380800 20261104.1803 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.94 19:31:11.12 +26:10:51.4
60.59136 3.63276 galactic Vul Second-epoch detections are separated by 0.6" and 7.0 pix
The object was found in VSX 3" ASASSN-V J193110.96+261053.5
Type: SR
# Max. Min./Amp. JD0 Period
14.530 V 14.910 V 2457845.10000 77.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:31:11.12 +26:10:51.4: 14.06 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:31:11.12 +26:10:51.4: 14.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193110.96+261053.5,2461348.6803,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193110.96+261053.5 20261104.1803 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.35 19:12:05.80 +26:43:15.3
59.08597 7.67022 galactic Lyr Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 3" EH Lyr
Type: L
# Max. Min./Amp. JD0 Period
13.900 pg 14.900 pg
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:05.80 +26:43:15.3: 12.29 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:05.80 +26:43:15.3: 12.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EH Lyr,2461348.6803,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EH Lyr 20261104.1803 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.95 19:12:07.45 +18:44:50.5
51.94427 4.04762 galactic Sge Second-epoch detections are separated by 1.8" and 7.3 pix
The object was found in VSX 1" ASASSN-V J191207.43+184450.1
Type: SR
# Max. Min./Amp. JD0 Period
15.960 g Y 0.500 g 2458582.88300 41.070000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:07.45 +18:44:50.5: 13.97 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:07.45 +18:44:50.5: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191207.43+184450.1,2461348.6803,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191207.43+184450.1 20261104.1803 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.57 19:22:00.22 +20:16:29.2
54.38148 2.69370 galactic Vul Second-epoch detections are separated by 0.9" and 7.3 pix
The object was found in VSX 1" ASASSN-V J192200.17+201629.6
Type: SRS
# Max. Min./Amp. JD0 Period
15.250 V 15.450 V 2457092.11000 22.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:22:00.22 +20:16:29.2: 14.69 +/- 0.11 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:22:00.22 +20:16:29.2: 14.59 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.64 +/- 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
ASASSN-V J192200.17+201629.6,2461348.6803,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192200.17+201629.6 20261104.1803 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.96 19:04:36.17 +24:48:39.8
56.60179 8.33521 galactic Vul Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX 2" ZTF J190436.04+244840.8
Type: SR
# Max. Min./Amp. JD0 Period
16.404 g Y 0.454 g 2458281.21910 138.574528700000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:36.17 +24:48:39.8: 13.93 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:36.17 +24:48:39.8: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190436.04+244840.8,2461348.6803,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190436.04+244840.8 20261104.1803 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.10 19:30:53.51 +26:39:50.1
60.98520 3.92110 galactic Vul Second-epoch detections are separated by 1.5" and 7.1 pix
The object was found in VSX 3" ASASSN-V J193053.51+263952.7
Type: SR
# Max. Min./Amp. JD0 Period
14.490 V 14.780 V 2458277.19320 85.093961600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:30:53.51 +26:39:50.1: 13.99 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:30:53.51 +26:39:50.1: 14.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193053.51+263952.7,2461348.6803,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193053.51+263952.7 20261104.1803 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.33 19:23:14.09 +24:27:38.1
58.22041 4.40313 galactic Vul Second-epoch detections are separated by 0.5" and 7.1 pix
The object was found in VSX 2" V0335 Vul
Type: M
# Max. Min./Amp. JD0 Period
11.500 V 13.900 V 2458553.68330 379.890349300000 C
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:23:14.09 +24:27:38.1: 12.22 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:23:14.09 +24:27:38.1: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0335 Vul,2461348.6803,11.33,0.05,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
V0335 Vul 20261104.1803 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 11 04.1803 2461348.6803 13.05 19:22:04.22 +20:14:03.6
54.35307 2.66091 galactic Vul Second-epoch detections are separated by 2.1" and 7.1 pix
The object was found in VSX 6" ZTF J192203.83+201400.6
Type: SR
# Max. Min./Amp. JD0 Period
17.154 g Y 0.421 g 2458322.84390 74.593918100000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:22:04.22 +20:14:03.6: 14.06 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:22:04.22 +20:14:03.6: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192203.83+201400.6,2461348.6803,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192203.83+201400.6 20261104.1803 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.97 19:23:07.44 +19:28:30.4
53.79906 2.08524 galactic Vul Second-epoch detections are separated by 2.2" and 7.5 pix
The object was found in VSX 1" ASASSN-V J192307.44+192831.3
Type: SR
# Max. Min./Amp. JD0 Period
14.430 V 14.600 V 2457205.83600 30.340000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:23:07.44 +19:28:30.4: 13.93 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:23:07.44 +19:28:30.4: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192307.44+192831.3,2461348.6803,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192307.44+192831.3 20261104.1803 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.98 19:18:23.45 +20:44:33.1
54.40025 3.66018 galactic Sge Second-epoch detections are separated by 0.3" and 7.3 pix
The object was found in VSX 1" ASASSN-V J191823.47+204433.6
Type: SR
# Max. Min./Amp. JD0 Period
14.650 V 14.790 V 2458370.00000 175.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:18:23.45 +20:44:33.1: 13.93 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:18:23.45 +20:44:33.1: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191823.47+204433.6,2461348.6803,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191823.47+204433.6 20261104.1803 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.85 19:05:16.09 +22:51:13.2
54.89772 7.33286 galactic Vul Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX 2" ASASSN-V J190516.06+225115.2
Type: L
# Max. Min./Amp. JD0 Period
14.080 V 14.410 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:05:16.09 +22:51:13.2: 13.93 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:05:16.09 +22:51:13.2: 13.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190516.06+225115.2,2461348.6803,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190516.06+225115.2 20261104.1803 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.59 19:24:22.28 +22:48:54.0
56.88601 3.40145 galactic Vul Second-epoch detections are separated by 2.2" and 7.6 pix
The object was found in VSX 2" ZTF J192422.38+224853.6
Type: SR
# Max. Min./Amp. JD0 Period
13.842 r Y 0.204 r 2458642.19200 46.974172000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:24:22.28 +22:48:54.0: 14.70 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:24:22.28 +22:48:54.0: 14.88 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.78 +/- 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
ZTF J192422.38+224853.6,2461348.6803,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192422.38+224853.6 20261104.1803 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.96 19:07:35.33 +19:51:27.0
52.44684 5.50592 galactic Sge Second-epoch detections are separated by 2.2" and 7.8 pix
The object was found in VSX 2" Gaia DR3 4519389438988273920
Type: L
# Max. Min./Amp. JD0 Period
12.860 G 13.010 G M
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:07:35.33 +19:51:27.0: 13.96 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:07:35.33 +19:51:27.0: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4519389438988273920,2461348.6803,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4519389438988273920 20261104.1803 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.00 19:20:10.34 +20:06:48.5
54.03735 2.99787 galactic Sge Second-epoch detections are separated by 1.5" and 7.5 pix
The object was found in VSX 1" ASASSN-V J192010.42+200649.0
Type: SR
# Max. Min./Amp. JD0 Period
14.700 V 14.840 V 2457559.00000 471.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:20:10.34 +20:06:48.5: 13.94 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:20:10.34 +20:06:48.5: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192010.42+200649.0,2461348.6803,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192010.42+200649.0 20261104.1803 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.96 19:14:22.83 +22:22:29.7
55.42216 5.24009 galactic Vul Second-epoch detections are separated by 1.0" and 7.1 pix
The object was found in VSX 5" ASASSN-V J191422.91+222234.6
Type: SRS
# Max. Min./Amp. JD0 Period
14.390 V 14.550 V 2457107.09000 24.201000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:14:22.83 +22:22:29.7: 13.90 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:14:22.83 +22:22:29.7: 13.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191422.91+222234.6,2461348.6803,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191422.91+222234.6 20261104.1803 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 11.13 18:55:46.19 +22:42:45.2
53.79905 9.23838 galactic Her Second-epoch detections are separated by 0.6" and 7.5 pix
The object was found in VSX 3" NSVS J1855457+224246
Type: SR
# Max. Min./Amp. JD0 Period
13.600 g Y 0.460 g 2458382.03720 60.446992800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:55:46.19 +22:42:45.2: 12.07 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:55:46.19 +22:42:45.2: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 55 46.19 +22 42 45.2 11.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1855457+224246,2461348.6803,11.13,0.05,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
NSVS J1855457+224246 20261104.1803 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 11 04.1803 2461348.6803 13.46 19:12:04.80 +18:50:25.1
52.02226 4.09954 galactic Sge Second-epoch detections are separated by 1.9" and 7.5 pix
The object was found in VSX 0" ASASSN-V J191204.81+185025.3
Type: SR
# Max. Min./Amp. JD0 Period
15.200 V 16.100 V 2458359.51240 147.428018200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:04.80 +18:50:25.1: 14.72 +/- 0.12 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:04.80 +18:50:25.1: 14.81 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191204.81+185025.3,2461348.6803,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191204.81+185025.3 20261104.1803 13.46CV 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 11 04.1803 2461348.6803 12.88 18:54:10.89 +21:29:23.6
52.52145 9.04038 galactic Her Second-epoch detections are separated by 0.8" and 7.7 pix
The object was found in VSX 2" ASASSN-V J185410.76+212922.4
Type: SR
# Max. Min./Amp. JD0 Period
15.759 g Y 1.084 g 2458590.66950 179.237042500000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:54:10.89 +21:29:23.6: 13.99 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:54:10.89 +21:29:23.6: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 54 10.89 +21 29 23.6 12.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185410.76+212922.4,2461348.6803,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185410.76+212922.4 20261104.1803 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.01 19:01:55.84 +19:53:52.5
51.88252 6.71273 galactic Sge Second-epoch detections are separated by 5.5" and 8.0 pix
The object was found in VSX 4" ASASSN-V J190155.72+195356.2
Type: SR
# Max. Min./Amp. JD0 Period
14.300 V 14.540 V 2457825.00000 758.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:01:55.84 +19:53:52.5: 14.01 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:01:55.84 +19:53:52.5: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190155.72+195356.2,2461348.6803,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190155.72+195356.2 20261104.1803 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.28 19:08:11.28 +22:28:15.7
54.85615 6.55927 galactic Vul Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX 2" ZTF J190811.12+222815.7
Type: SR
# Max. Min./Amp. JD0 Period
14.107 r Y 0.444 r 2458297.69540 226.248561800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:08:11.28 +22:28:15.7: 14.71 +/- 0.13 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:08:11.28 +22:28:15.7: 14.90 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.77 +/- 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
ZTF J190811.12+222815.7,2461348.6803,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190811.12+222815.7 20261104.1803 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.80 19:15:27.07 +24:45:21.9
57.66368 6.10898 galactic Vul Second-epoch detections are separated by 1.5" and 7.5 pix
The object was found in VSX 1" ASASSN-V J191527.02+244520.6
Type: SR
# Max. Min./Amp. JD0 Period
14.150 V 14.460 V 2458233.00000 322.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:15:27.07 +24:45:21.9: 13.91 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:15:27.07 +24:45:21.9: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191527.02+244520.6,2461348.6803,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191527.02+244520.6 20261104.1803 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 10.90 19:00:27.72 +24:43:46.3
56.11186 9.14496 galactic Vul Second-epoch detections are separated by 0.2" and 7.4 pix
The object was found in VSX 0" ASAS J190028+2443.8
Type: MISC
# Max. Min./Amp. JD0 Period
8.477 Ic Y 0.546 Ic 2452754.10000 211.200000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:00:27.72 +24:43:46.3: 12.13 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:00:27.72 +24:43:46.3: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 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
ASAS J190028+2443.8,2461348.6803,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190028+2443.8 20261104.1803 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.79 19:46:47.03 +18:01:59.9
55.26056 -3.51029 galactic Sge Second-epoch detections are separated by 1.2" and 7.2 pix
The object was found in VSX 1" ZTF J194647.03+180201.1
Type: M
# Max. Min./Amp. JD0 Period
16.280 r Y 4.845 r 2458387.31230 400.758677500000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:46:47.03 +18:01:59.9: 13.95 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:46:47.03 +18:01:59.9: 13.83 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194647.03+180201.1,2461348.6803,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194647.03+180201.1 20261104.1803 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.84 19:03:43.93 +25:59:04.1
57.58168 9.02605 galactic Lyr Second-epoch detections are separated by 1.4" and 7.5 pix
The object was found in VSX 5" ASASSN-V J190343.76+255908.4
Type: SR
# Max. Min./Amp. JD0 Period
14.130 V 14.710 V 2457180.90000 60.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:03:43.93 +25:59:04.1: 13.85 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:03:43.93 +25:59:04.1: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190343.76+255908.4,2461348.6803,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190343.76+255908.4 20261104.1803 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 10.78 18:50:51.69 +20:11:21.2
50.99389 9.17618 galactic Her Second-epoch detections are separated by 0.5" and 7.6 pix
The object was found in VSX 6" NSVS J1850515+201130
Type: SR
# Max. Min./Amp. JD0 Period
13.623 g Y 0.554 g 2458358.88660 264.200904400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:50:51.69 +20:11:21.2: 11.82 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:50:51.69 +20:11:21.2: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 50 51.69 +20 11 21.2 10.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1850515+201130,2461348.6803,10.78,0.05,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
NSVS J1850515+201130 20261104.1803 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 11 04.1803 2461348.6803 12.83 19:09:56.06 +22:44:17.5
55.27880 6.31960 galactic Vul Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX 1" ASASSN-V J190956.02+224418.7
Type: L:
# Max. Min./Amp. JD0 Period
13.760 V 14.040 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:56.06 +22:44:17.5: 13.86 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:56.06 +22:44:17.5: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190956.02+224418.7,2461348.6803,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190956.02+224418.7 20261104.1803 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.82 19:06:44.52 +23:13:33.0
55.38585 7.19500 galactic Vul Second-epoch detections are separated by 0.7" and 7.5 pix
The object was found in VSX 1" ASASSN-V J190644.44+231333.9
Type: SR
# Max. Min./Amp. JD0 Period
13.122 r Y 0.610 r 2458353.71490 90.198107900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:06:44.52 +23:13:33.0: 13.92 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:06:44.52 +23:13:33.0: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190644.44+231333.9,2461348.6803,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190644.44+231333.9 20261104.1803 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.84 19:39:20.36 +26:34:31.1
61.82248 2.22599 galactic Vul Second-epoch detections are separated by 1.8" and 7.3 pix
The object was found in VSX 5" ASASSN-V J193920.62+263435.3
Type: SR
# Max. Min./Amp. JD0 Period
14.380 V 14.970 V 2458344.26390 68.636266200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:39:20.36 +26:34:31.1: 13.76 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:39:20.36 +26:34:31.1: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193920.62+263435.3,2461348.6803,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193920.62+263435.3 20261104.1803 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.91 19:48:11.32 +26:43:32.3
62.93802 0.58629 galactic Vul Second-epoch detections are separated by 3.1" and 6.7 pix
The object was found in VSX 5" NSVS 8389420
Type: SR
# Max. Min./Amp. JD0 Period
16.961 g Y 0.450 R1 2458638.51120 96.742503400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:48:11.32 +26:43:32.3: 13.89 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:48:11.32 +26:43:32.3: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8389420,2461348.6803,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8389420 20261104.1803 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.40 19:20:38.86 +19:09:45.6
53.24839 2.45426 galactic Sge Second-epoch detections are separated by 1.9" and 7.2 pix
The object was found in VSX 1" ZTF J192038.93+190945.6
Type: SR
# Max. Min./Amp. JD0 Period
13.709 r Y 0.302 r 2458334.96160 62.328210200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:20:38.86 +19:09:45.6: 14.65 +/- 0.11 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:20:38.86 +19:09:45.6: 14.58 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.61 +/- 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
ZTF J192038.93+190945.6,2461348.6803,13.40,0.05,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
ZTF J192038.93+190945.6 20261104.1803 13.40CV 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 11 04.1803 2461348.6803 13.33 19:09:45.51 +24:01:34.9
56.41872 6.93515 galactic Vul Second-epoch detections are separated by 1.9" and 7.2 pix
The object was found in VSX 1" ASASSN-V J190945.60+240135.3
Type: SR
# Max. Min./Amp. JD0 Period
14.740 V 15.390 V 2457695.70000 431.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:45.51 +24:01:34.9: 14.67 +/- 0.12 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:45.51 +24:01:34.9: 14.76 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190945.60+240135.3,2461348.6803,13.33,0.05,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
ASASSN-V J190945.60+240135.3 20261104.1803 13.33CV 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 11 04.1803 2461348.6803 12.85 19:04:45.78 +26:35:53.3
58.24291 9.08588 galactic Lyr Second-epoch detections are separated by 2.2" and 7.1 pix
The object was found in VSX 5" NSVS J1904456+263557
Type: SR
# Max. Min./Amp. JD0 Period
16.044 g Y 0.922 g 2458419.49510 282.234274400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:45.78 +26:35:53.3: 13.81 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:45.78 +26:35:53.3: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1904456+263557,2461348.6803,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1904456+263557 20261104.1803 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.78 19:09:59.05 +26:11:25.6
58.39392 7.85666 galactic Lyr Second-epoch detections are separated by 0.8" and 7.3 pix
The object was found in VSX 4" ASASSN-V J190958.79+261126.9
Type: SR
# Max. Min./Amp. JD0 Period
14.960 g Y 0.380 g 2458731.53700 598.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:09:59.05 +26:11:25.6: 13.79 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:09:59.05 +26:11:25.6: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190958.79+261126.9,2461348.6803,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190958.79+261126.9 20261104.1803 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.79 19:24:07.20 +23:59:24.5
57.89837 4.00452 galactic Vul Second-epoch detections are separated by 1.9" and 7.1 pix
The object was found in VSX 3" ASASSN-V J192407.23+235927.2
Type: SR
# Max. Min./Amp. JD0 Period
14.430 V 14.610 V 2457231.97000 39.150000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:24:07.20 +23:59:24.5: 13.79 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:24:07.20 +23:59:24.5: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192407.23+235927.2,2461348.6803,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192407.23+235927.2 20261104.1803 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.89 19:16:30.20 +25:16:30.4
58.23757 6.13354 galactic Vul Second-epoch detections are separated by 2.9" and 6.9 pix
The object was found in VSX 4" ASASSN-V J191630.03+251633.0
Type: SR
# Max. Min./Amp. JD0 Period
14.110 V 14.370 V 2458284.22500 154.554587400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:16:30.20 +25:16:30.4: 13.84 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:16:30.20 +25:16:30.4: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191630.03+251633.0,2461348.6803,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191630.03+251633.0 20261104.1803 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.31 19:08:35.55 +19:29:07.5
52.22122 5.12671 galactic Sge Second-epoch detections are separated by 1.4" and 7.6 pix
The object was found in VSX 1" ASASSN-V J190835.61+192908.3
Type: SR
# Max. Min./Amp. JD0 Period
15.000 V 15.600 V 2457133.00000 74.900000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:08:35.55 +19:29:07.5: 14.75 +/- 0.14 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:08:35.55 +19:29:07.5: 14.88 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190835.61+192908.3,2461348.6803,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190835.61+192908.3 20261104.1803 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 10.33 19:02:36.44 +21:09:36.7
53.09224 7.13259 galactic Sge Second-epoch detections are separated by 1.7" and 7.5 pix
The object was found in VSX 1" ASAS J190236+2109.6
Type: MISC
# Max. Min./Amp. JD0 Period
11.723 V Y 0.405 V 1.012836000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:02:36.44 +21:09:36.7: 11.31 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:02:36.44 +21:09:36.7: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190236+2109.6,2461348.6803,10.33,0.05,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
ASAS J190236+2109.6 20261104.1803 10.33CV 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 11 04.1803 2461348.6803 12.73 19:13:43.42 +18:52:08.2
52.22687 3.76731 galactic Sge Second-epoch detections are separated by 1.8" and 7.6 pix
The object was found in VSX 1" ASASSN-V J191343.44+185207.7
Type: SR
# Max. Min./Amp. JD0 Period
14.380 V 14.840 V 2458330.18560 76.462960900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:13:43.42 +18:52:08.2: 13.79 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:13:43.42 +18:52:08.2: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191343.44+185207.7,2461348.6803,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191343.44+185207.7 20261104.1803 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.27 19:05:02.23 +18:38:05.2
51.07763 5.49106 galactic Aql Second-epoch detections are separated by 1.8" and 7.8 pix
The object was found in VSX 3" ASASSN-V J190502.03+183806.9
Type: SR
# Max. Min./Amp. JD0 Period
14.630 V 15.160 V 2458377.63910 66.974993600000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:05:02.23 +18:38:05.2: 14.65 +/- 0.14 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:05:02.23 +18:38:05.2: 14.53 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.59 +/- 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
ASASSN-V J190502.03+183806.9,2461348.6803,13.27,0.05,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
ASASSN-V J190502.03+183806.9 20261104.1803 13.27CV 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 11 04.1803 2461348.6803 12.87 19:16:20.28 +26:21:24.3
59.18948 6.65932 galactic Lyr Second-epoch detections are separated by 0.3" and 7.2 pix
The object was found in VSX 3" ASASSN-V J191620.31+262127.0
Type: SR
# Max. Min./Amp. JD0 Period
13.950 V 14.370 V 2458632.81250 77.948184400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:16:20.28 +26:21:24.3: 13.77 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:16:20.28 +26:21:24.3: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191620.31+262127.0,2461348.6803,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191620.31+262127.0 20261104.1803 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.87 19:22:11.80 +17:44:10.2
52.16076 1.46013 galactic Sge Second-epoch detections are separated by 1.3" and 7.4 pix
The object was found in VSX 1" ASASSN-V J192211.76+174409.8
Type: L
# Max. Min./Amp. JD0 Period
15.860 g Y 0.340 g 2459439.54000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:22:11.80 +17:44:10.2: 13.81 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:22:11.80 +17:44:10.2: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192211.76+174409.8,2461348.6803,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192211.76+174409.8 20261104.1803 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.45 19:05:42.92 +20:31:51.8
52.85212 6.20188 galactic Sge Second-epoch detections are separated by 5.2" and 8.3 pix
The object was found in VSX 4" ZTF J190542.72+203154.2
Type: SR
# Max. Min./Amp. JD0 Period
16.037 g Y 0.110 g 2458271.89540 28.923168800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:05:42.92 +20:31:51.8: 14.66 +/- 0.11 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:05:42.92 +20:31:51.8: 14.49 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.57 +/- 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
ZTF J190542.72+203154.2,2461348.6803,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190542.72+203154.2 20261104.1803 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.76 18:51:42.33 +20:47:54.9
51.63710 9.26153 galactic Her Second-epoch detections are separated by 1.1" and 7.7 pix
The object was found in VSX 2" ASASSN-V J185142.18+204755.4
Type: SR
# Max. Min./Amp. JD0 Period
16.330 g Y 1.010 g 2459535.54700 88.030000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:51:42.33 +20:47:54.9: 13.82 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:51:42.33 +20:47:54.9: 13.78 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 04.1803* 18 51 42.33 +20 47 54.9 12.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185142.18+204755.4,2461348.6803,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185142.18+204755.4 20261104.1803 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.72 19:01:16.48 +18:03:00.1
50.14932 6.02586 galactic Aql Second-epoch detections are separated by 1.4" and 7.6 pix
The object was found in VSX 1" NSVS 11188832
Type: SR
# Max. Min./Amp. JD0 Period
16.543 g Y 0.550 R1 2458212.80700 181.545716000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:01:16.48 +18:03:00.1: 13.80 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:01:16.48 +18:03:00.1: 13.82 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11188832,2461348.6803,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11188832 20261104.1803 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.41 19:05:07.40 +22:24:35.3
54.48203 7.16528 galactic Vul Second-epoch detections are separated by 2.2" and 7.1 pix
The object was found in VSX 2" ZTF J190507.29+222435.8
Type: SR
# Max. Min./Amp. JD0 Period
14.536 r Y 0.409 r 2458274.32020 65.576682200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:05:07.40 +22:24:35.3: 14.56 +/- 0.10 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:05:07.40 +22:24:35.3: 14.78 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.66 +/- 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
ZTF J190507.29+222435.8,2461348.6803,13.41,0.05,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
ZTF J190507.29+222435.8 20261104.1803 13.41CV 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 11 04.1803 2461348.6803 13.53 19:12:40.49 +20:26:28.9
53.51402 4.70847 galactic Sge Second-epoch detections are separated by 0.6" and 7.3 pix
The object was found in VSX 1" NSVS 11206344
Type: SR
# Max. Min./Amp. JD0 Period
12.700 R1 13.300 R1 2451486.00000 100.000000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:40.49 +20:26:28.9: 14.59 +/- 0.11 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:40.49 +20:26:28.9: 14.53 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.56 +/- 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
NSVS 11206344,2461348.6803,13.53,0.05,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
NSVS 11206344 20261104.1803 13.53CV 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 11 04.1803 2461348.6803 12.84 19:23:42.39 +22:27:26.1
56.49747 3.36861 galactic Vul Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 2" ASASSN-V J192342.41+222728.0
Type: SR
# Max. Min./Amp. JD0 Period
13.970 V 14.630 V 2457600.00000 372.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:23:42.39 +22:27:26.1: 13.76 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:23:42.39 +22:27:26.1: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192342.41+222728.0,2461348.6803,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192342.41+222728.0 20261104.1803 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.86 19:16:46.42 +22:16:41.1
55.59084 4.70396 galactic Vul Second-epoch detections are separated by 2.0" and 7.6 pix
The object was found in VSX 0" ZTF J191646.38+221641.4
Type: SR
# Max. Min./Amp. JD0 Period
15.407 g Y 0.258 g 2458581.91160 39.385268200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:16:46.42 +22:16:41.1: 13.73 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:16:46.42 +22:16:41.1: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191646.38+221641.4,2461348.6803,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191646.38+221641.4 20261104.1803 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.78 19:16:56.80 +21:23:28.5
54.82017 4.25923 galactic Vul Second-epoch detections are separated by 0.6" and 7.4 pix
The object was found in VSX 1" ASASSN-V J191656.74+212328.2
Type: SR
# Max. Min./Amp. JD0 Period
17.580 g Y 1.320 g 2459472.48500 81.800000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:16:56.80 +21:23:28.5: 13.72 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:16:56.80 +21:23:28.5: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191656.74+212328.2,2461348.6803,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191656.74+212328.2 20261104.1803 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 12.46 18:50:58.78 +20:11:35.6
51.00970 9.15292 galactic Her Second-epoch detections are separated by 0.4" and 7.5 pix
The object was found in VSX 4" ASASSN-V J185058.51+201135.3
Type: L
# Max. Min./Amp. JD0 Period
14.090 V 14.600 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:50:58.78 +20:11:35.6: 13.74 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:50:58.78 +20:11:35.6: 13.61 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 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!
TCP 2026 11 04.1803* 18 50 58.78 +20 11 35.6 12.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185058.51+201135.3,2461348.6803,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185058.51+201135.3 20261104.1803 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 11 04.1803 2461348.6803 12.82 19:22:01.80 +19:17:34.6
53.51673 2.22719 galactic Sge Second-epoch detections are separated by 1.5" and 7.5 pix
The object was found in VSX15" Gaia DR3 4515732257150423296
Type: L
# Max. Min./Amp. JD0 Period
17.790 G 17.930 G
ATTENTION: measured mag 12.82 is 5.0 mag brighter than the VSX record maximum brightness 17.79 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:22:01.80 +19:17:34.6: 13.75 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:22:01.80 +19:17:34.6: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 4515732257150423296,2461348.6803,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4515732257150423296 20261104.1803 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.57 19:24:47.32 +20:32:41.6
54.92758 2.24526 galactic Vul Second-epoch detections are separated by 3.0" and 7.0 pix
The object was found in VSX 2" ZTF J192447.37+203243.7
Type: SR
# Max. Min./Amp. JD0 Period
13.977 r Y 0.139 r 2458269.79280 41.287769500000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:24:47.32 +20:32:41.6: 14.56 +/- 0.09 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:24:47.32 +20:32:41.6: 14.87 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192447.37+203243.7,2461348.6803,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192447.37+203243.7 20261104.1803 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 04.1803 2461348.6803 13.32 19:07:00.45 +20:14:09.9
52.72430 5.79872 galactic Sge Second-epoch detections are separated by 1.2" and 7.5 pix
The object was found in VSX 1" ASASSN-V J190700.46+201411.3
Type: SR
# Max. Min./Amp. JD0 Period
14.760 V 15.080 V 2457099.00000 524.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:07:00.45 +20:14:09.9: 14.54 +/- 0.11 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:07:00.45 +20:14:09.9: 14.49 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190700.46+201411.3,2461348.6803,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190700.46+201411.3 20261104.1803 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.93408543 17.05.2026 10:24:54.981 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
First image: 2461177.93408543 17.05.2026 10:24:54.981 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Last image: 2461348.68065634 04.11.2026 04:19:58.708 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 26290
Objects passed selection criteria: 26237
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 22456.2
Average stars matched: 21828.8 (97.2057 %)
Memory usage VmPeak: 250132 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 22:25:50 CST 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: 2461177.93408543 17.05.2026 10:24:54.981 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
First image: 2461177.93408543 17.05.2026 10:24:54.981 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Last image: 2461348.68065634 04.11.2026 04:19:58.708 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 883
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.15
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: 105 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 210720
Objects passed selection criteria: 210179
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 164533
Average stars matched: 157286 (95.5954 %)
Memory usage VmPeak: 669560 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 22:28:37 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
SExtractor catalog cache: saved Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.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/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461348.68002916
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_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits exists and is non-empty
wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits exists and is non-empty
wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits exists and is non-empty
wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits (1st reference image)
verification OK: wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:23:04.844 +22:00:37.34 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits (1st new image)
verification OK: wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:23:04.966 +22:00:07.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:23:04.844 +22:00:37.34
Second-epoch image center 19:23:04.966 +22:00:07.71
Angular distance between the image centers 0.0082 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits (2nd new image)
verification OK: wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:23:02.323 +22:00:30.75 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:23:04.844 +22:00:37.34
Second-epoch image center 19:23:02.323 +22:00:30.75
Angular distance between the image centers 0.0099 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 19:23:04.966 +22:00:07.71
Second-epoch second image center 19:23:02.323 +22:00:30.75
Angular distance between the image centers 0.01205 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits &> /tmp/tmp.jh6fUktxs1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits &> /tmp/tmp.cEmcHhVWtQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits &> /tmp/tmp.xsMgoobdbq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits &> /tmp/tmp.hOfFUPNICl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.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_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits and wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits and wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat
Found non-empty wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits and wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat
The reference image (wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits) and catalog (wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat) found
'wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat' -> 'wcsmag.cat'
Read 27697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 282.0063 to 299.5194 deg, Dec +16.5860 to +27.2738 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 282.0063 to 299.5194 deg, Dec 16.5860 to 27.2738 deg
Loaded 18856 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): 13417 out of 14659 total matches.
Matched with Tycho-2 14659 out of 27697 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749000
a=0.000000 b=1.000000 c=22.749000
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 282.0063 to 299.5194 deg, Dec +16.5860 to +27.2738 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 282.0063 to 299.5194 deg, Dec 16.5860 to 27.2738 deg
Loaded 18856 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): 13417 out of 14659 total matches.
Matched with Tycho-2 14659 out of 27697 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Forced-photometry filter: calibrated wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits -> calib.txt_param_ref_wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits (aperture=6.4)
Read 27510 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 282.0063 to 299.5197 deg, Dec +16.5985 to +27.2882 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 282.0063 to 299.5197 deg, Dec 16.5985 to 27.2882 deg
Loaded 18878 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): 13378 out of 14613 total matches.
Matched with Tycho-2 14613 out of 27510 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Forced-photometry filter: calibrated wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits -> calib.txt_param_ref_wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
2.4 pix Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
4.9 pix fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
4.9 pix fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
Limiting magnitude estimates:
15.3 mag. Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
15.3 mag. Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
14.3 mag. fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
14.3 mag. fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.jh6fUktxs1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits' -> 'wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WCS-calibrated image found: wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Checking if the catalog wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat corresponding to the image wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat corresponding to the image wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WCS catalog name: wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2722, bad_region=0, passed=27697
Got 27697 stars (including 24942 good ones) from the SExtractor catalog wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat
util/solve_plate_with_UCAC5 got 27697 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 4920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 27697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 27697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 27697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 4920 stars left (next iteration limit 5412)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits N_match=4920 sigma_overall_arcsec=0.644 sigma_q1_arcsec=0.481 sigma_q2_arcsec=0.917 sigma_q3_arcsec=0.547 sigma_q4_arcsec=0.647 n_q1=1047 n_q2=1444 n_q3=1119 n_q4=1310 worst_quadrant_to_overall_ratio=1.423
WCS_HEADER_DIAG: file=Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits selection=current_pairs N_selected=4920 N_valid=4920 bias_ra_arcsec=0.028 bias_dec_arcsec=-0.002 median_sep_arcsec=0.425 p95_sep_arcsec=3.101 n_q1=1047 n_q2=1444 n_q3=1119 n_q4=1310 occupied_cells_4x4=16/16
The image catalog is written to wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits -region wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.cEmcHhVWtQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits' -> 'wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WCS-calibrated image found: wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Checking if the catalog wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.wcscat corresponding to the image wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.wcscat corresponding to the image wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WCS catalog name: wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2737, bad_region=0, passed=27506
Got 27506 stars (including 24749 good ones) from the SExtractor catalog wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.wcscat
util/solve_plate_with_UCAC5 got 27506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 4911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 27506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 27506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 27506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 4913 stars left (next iteration limit 5402)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits N_match=4913 sigma_overall_arcsec=0.632 sigma_q1_arcsec=0.469 sigma_q2_arcsec=0.910 sigma_q3_arcsec=0.569 sigma_q4_arcsec=0.626 n_q1=1047 n_q2=1437 n_q3=1123 n_q4=1306 worst_quadrant_to_overall_ratio=1.438
WCS_HEADER_DIAG: file=Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits selection=current_pairs N_selected=4913 N_valid=4913 bias_ra_arcsec=0.043 bias_dec_arcsec=-0.002 median_sep_arcsec=0.436 p95_sep_arcsec=3.157 n_q1=1047 n_q2=1437 n_q3=1123 n_q4=1306 occupied_cells_4x4=16/16
The image catalog is written to wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits -region wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.xsMgoobdbq (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_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.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_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
Checking if the catalog wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat corresponding to the image wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat corresponding to the image wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
WCS catalog name: wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=955, bad_region=3, passed=17397
Got 17397 stars (including 16427 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat
util/solve_plate_with_UCAC5 got 17397 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 17397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 17397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 17397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 4901 stars left (next iteration limit 5388)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4901 robust_rms=13.625 arcsec worst_region_rms=24.901 arcsec outer_annulus_rms=24.901 arcsec
SIP_REFIT: SIP order 3 trial: matched=4901 robust_rms=0.749 arcsec worst_region_rms=1.228 arcsec outer_annulus_rms=1.228 arcsec
SIP_REFIT: SIP order 5 trial: matched=4901 robust_rms=0.686 arcsec worst_region_rms=1.107 arcsec outer_annulus_rms=1.107 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4901 robust_rms_before=1.520 arcsec robust_rms_before_corrected=0.789 arcsec robust_rms_after=0.686 arcsec worst_region_rms_before=1.268 worst_region_rms_after=1.107 outer_annulus_rms_before=2.269 outer_annulus_rms_after=1.107
verification OK: wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.sip_refit.fwdbKk/candidate.fits
verification OK: wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.sip_refit.fwdbKk/candidate.fits
Image size: 941.7'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:23:04.966 +22:00:07.11 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 17397 stars ###
'wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.sip_refit.fwdbKk/candidate.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction_2588632.cat.log'
'wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.sip_refit.fwdbKk/candidate.wcscat.xy2sky.Tp81d6' -> 'vast_debug_catalog_after_xy2sky_correction_2588632.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.520 -> 0.686 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.4 arcsec, 4901 pairs from the previous matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4628 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4628 pairs (4901 from the previous matching)
SIP_REFIT: SIP order 2 trial: matched=4628 robust_rms=13.273 arcsec worst_region_rms=24.334 arcsec outer_annulus_rms=24.334 arcsec
SIP_REFIT: SIP order 3 trial: matched=4628 robust_rms=0.735 arcsec worst_region_rms=1.168 arcsec outer_annulus_rms=1.168 arcsec
SIP_REFIT: SIP order 5 trial: matched=4628 robust_rms=0.665 arcsec worst_region_rms=1.073 arcsec outer_annulus_rms=1.073 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4628 robust_rms_before=0.665 arcsec robust_rms_before_corrected=0.665 arcsec robust_rms_after=0.665 arcsec worst_region_rms_before=1.055 worst_region_rms_after=1.073 outer_annulus_rms_before=1.055 outer_annulus_rms_after=1.073
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-region 1.073 vs 1.055 arcsec) - keeping the current solution
SIP_REFIT: the refit on the re-matched pairs was not applied - keeping the current solution
Accuracy estimation diagnostic: 4628 matched stars entering correct_measured_positions(), 17397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Accuracy estimation diagnostic: 4628 matched stars entering correct_measured_positions(), 17397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
WCS_QUALITY_DIAG: file=fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits N_match=4628 sigma_overall_arcsec=0.663 sigma_q1_arcsec=0.625 sigma_q2_arcsec=0.881 sigma_q3_arcsec=0.588 sigma_q4_arcsec=0.595 n_q1=1293 n_q2=1036 n_q3=1350 n_q4=949 worst_quadrant_to_overall_ratio=1.329
WCS_HEADER_DIAG: file=fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits selection=current_pairs N_selected=4628 N_valid=4628 bias_ra_arcsec=0.016 bias_dec_arcsec=0.007 median_sep_arcsec=0.534 p95_sep_arcsec=1.832 n_q1=1293 n_q2=1036 n_q3=1350 n_q4=949 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits -region wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hOfFUPNICl (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_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.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_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
Checking if the catalog wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat corresponding to the image wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat corresponding to the image wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
WCS catalog name: wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1012, bad_region=0, passed=17988
Got 17988 stars (including 16967 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat
util/solve_plate_with_UCAC5 got 17988 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 4898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 17988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 17988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 17988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 4897 stars left (next iteration limit 5385)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4897 robust_rms=13.691 arcsec worst_region_rms=24.552 arcsec outer_annulus_rms=24.552 arcsec
SIP_REFIT: SIP order 3 trial: matched=4897 robust_rms=0.739 arcsec worst_region_rms=1.229 arcsec outer_annulus_rms=1.229 arcsec
SIP_REFIT: SIP order 5 trial: matched=4897 robust_rms=0.665 arcsec worst_region_rms=1.118 arcsec outer_annulus_rms=1.118 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4897 robust_rms_before=1.553 arcsec robust_rms_before_corrected=0.779 arcsec robust_rms_after=0.665 arcsec worst_region_rms_before=1.241 worst_region_rms_after=1.118 outer_annulus_rms_before=2.334 outer_annulus_rms_after=1.118
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 1.241 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits worst_region_rms_kept=1.241 arcsec robust_rms_kept=0.779 arcsec matched=4897
WCS_QUALITY_DIAG: file=fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits N_match=4897 sigma_overall_arcsec=0.732 sigma_q1_arcsec=0.728 sigma_q2_arcsec=0.994 sigma_q3_arcsec=0.621 sigma_q4_arcsec=0.672 n_q1=1342 n_q2=1112 n_q3=1457 n_q4=986 worst_quadrant_to_overall_ratio=1.358
WCS_HEADER_DIAG: file=fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits selection=current_pairs N_selected=4897 N_valid=4897 bias_ra_arcsec=-0.931 bias_dec_arcsec=0.365 median_sep_arcsec=1.373 p95_sep_arcsec=4.101 n_q1=1342 n_q2=1112 n_q3=1457 n_q4=986 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits -region wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits to local_wcs_cache/
'wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits' -> 'local_wcs_cache/wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits'
Saving the final (post-refit) wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits to local_wcs_cache/
'wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits' -> 'local_wcs_cache/wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits'
Saving the final (post-refit) wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits'
Saving the final (post-refit) wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits sigma_overall=0.644 worst_q_ratio=1.423
ref2=Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits sigma_overall=0.632 worst_q_ratio=1.438
new1=fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits sigma_overall=0.663 worst_q_ratio=1.329
new2=fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits sigma_overall=0.732 worst_q_ratio=1.358
reference average sigma_overall=0.638 worst_q_ratio=1.4305
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311_astrometric_residuals.png (4920 matched stars from wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312_astrometric_residuals.png (4913 matched stars from wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004_astrometric_residuals.png (4628 matched stars from wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005_astrometric_residuals.png (4897 matched stars from wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.70 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits'
Preparing the HTML report for the field Vul-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:56:25.68 +22:41:53.6: 11.99 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:57:23.85 +24:15:29.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:54:59.97 +25:14:03.1: 11.50 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:57:23.85 +24:15:29.2: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 19:57:23.85 +24:15:29.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:56:25.68 +22:41:53.6: 11.98 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:54:59.97 +25:14:03.1: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Forced photometry filter REJECTED candidate at 19:56:25.68 +22:41:53.6: ref_mag=11.98 +/- 0.01 new_mean_mag=11.8326 delta=0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:54:59.97 +25:14:03.1: ref_mag=11.50 +/- 0.01 new_mean_mag=11.5128 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:48:20.15 +21:11:00.4: 12.13 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:12:10.29 +24:18:34.5: 12.61 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:48:20.15 +21:11:00.4: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter REJECTED candidate at 19:48:20.15 +21:11:00.4: ref_mag=12.13 +/- 0.01 new_mean_mag=11.5999 delta=0.53 (need > 0.90)
Forced photometry on wcs_Vul-01-Q1b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:12:10.29 +24:18:34.5: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 19:12:10.29 +24:18:34.5: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6841 delta=0.90 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out32306.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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: 0s
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Considering the candidate 31726_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31726_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:54:01.49 +17:28:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31729_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31729_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:54:13.82 +19:15:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31730_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31730_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 31732_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31732_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:48:28.83 +17:00:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31733_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31733_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 31734_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31734_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:49.24 +18:44:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31735_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31735_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:53.10 +20:31:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31736_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31736_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:46.44 +18:46:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31751_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31751_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 31797_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31797_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:11.83 +26:00:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31901_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31901_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:12:42.73 +23:11:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31988_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31988_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 31990_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31990_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:35:45.68 +16:50:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32016_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32016_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:31:10.39 +23:30:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32023_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32023_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:11.11 +17:27:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32051_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32051_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:44.78 +18:26:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32060_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32060_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:58:30.26 +20:06:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32098_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32098_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:56.94 +22:04:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32120_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32120_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:57:37.09 +23:26:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32134_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32134_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:30.27 +21:22:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32147_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32147_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 32152_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32152_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:36:52.88 +25:19:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32164_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32164_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:58.98 +25:07:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32183_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32183_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:08.12 +19:00:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:25:51.34 +21:29:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32212_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32212_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:39:33.48 +19:43:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32213_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32213_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:58.53 +17:30:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32222_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32222_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:41:01.47 +16:56:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32235_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32235_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:45:37.71 +22:51:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32306_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32306_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:12:10.29 +24:18:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 1.477 2023370607977414528 288.04270798513 +24.30996425859 10.9376 9.5749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32341_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 32341_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:36:16.75 +18:52:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30907_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 30907_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:00.94 +18:02:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10220_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 10220_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:54.02 +20:17:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03299_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 03299_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:14.80 +17:45:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17731_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 17731_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265605_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265605_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265610_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265610_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265612_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 265612_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 265614_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265614_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265617_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265617_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265619_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265619_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265632_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265632_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 265658_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265658_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265665_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265665_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265676_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265676_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265677_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265677_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265678_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 265678_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 265684_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265684_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265688_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265688_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:36:38.79 +17:12:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265689_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265689_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265695_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265695_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265698_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265698_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265702_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265702_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265709_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265709_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265713_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265713_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265718_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265718_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265719_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265719_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265726_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265726_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265728_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265728_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265737_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265737_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265743_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265743_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265749_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265749_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 265758_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265758_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265763_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265763_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265771_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265771_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265774_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265774_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265775_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265775_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265778_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265778_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265782_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265782_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265783_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265783_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:42.31 +25:44:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265784_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265784_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265785_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265785_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265786_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265786_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265790_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265790_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265796_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265796_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:52:55.92 +19:26:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265797_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265797_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 265801_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265801_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:43:44.70 +18:08:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265803_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265803_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:54:34.66 +21:03:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265812_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265812_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:35.74 +17:37:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265813_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265813_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265815_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265815_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:52:44.45 +16:53:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265816_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265816_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 265832_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265832_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 265837_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265837_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:52:32.81 +17:52:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265845_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265845_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 265848_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265848_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:49.81 +16:59:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265854_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265854_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:52:15.88 +17:49:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265855_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265855_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265862_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265862_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265865_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265865_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265866_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265866_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265873_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265873_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265874_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265874_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265876_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265876_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265878_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265878_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265887_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265887_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265889_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265889_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:52:46.79 +17:25:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265900_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265900_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265906_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265906_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265908_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265908_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265909_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265909_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265913_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265913_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:57.07 +20:29:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265915_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265915_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265921_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265921_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265922_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265922_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:07.94 +16:59:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265926_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265926_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265930_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265930_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265934_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265934_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:30.61 +18:12:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265935_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265935_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265938_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265938_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265939_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265939_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:49:51.80 +16:56:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265943_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265943_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:49:27.88 +16:51:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265945_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265945_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:52:36.17 +17:31:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265946_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265946_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265949_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265949_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:54:13.46 +17:32:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265951_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265951_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:48:54.35 +17:30:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265954_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265954_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265955_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265955_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:48:34.88 +17:11:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265957_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265957_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265958_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265958_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 265961_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265961_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265963_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265963_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:31.56 +18:14:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265964_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265964_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:50:23.07 +17:39:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265965_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265965_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265966_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265966_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265967_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265967_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:55:15.25 +19:56:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265969_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265969_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265972_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265972_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265974_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265974_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:54:01.48 +17:28:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265976_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265976_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:50:18.04 +16:56:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265977_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265977_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:54:20.70 +17:52:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265979_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265979_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:02.84 +22:23:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265980_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265980_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265981_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265981_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265982_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265982_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:54:13.77 +19:15:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265984_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265984_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:48:28.85 +17:00:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265985_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265985_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 265986_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265986_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:49.30 +18:44:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265987_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 265987_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:53.11 +20:31:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266004_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266004_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 266082_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266082_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 266253_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266253_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:55:31.65 +23:04:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266266_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266266_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 266279_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266279_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:11.02 +17:27:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:03:42.34 +19:32:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266455_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 266455_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 266489_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266489_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:41:01.49 +16:56:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266551_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266551_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 266569_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266569_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:50:36.55 +17:15:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266630_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266630_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:58.73 +25:23:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266633_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266633_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:55:50.81 +25:00:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266655_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266655_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:32.72 +20:00:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266678_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266678_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:57:21.81 +18:53:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266686_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266686_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 266694_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266694_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 266703_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266703_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:14.67 +26:10:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266829_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266829_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:48:53.94 +19:06:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266863_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266863_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:57:17.37 +21:40:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266897_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266897_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 266941_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266941_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:30.89 +20:52:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266963_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266963_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:40:54.70 +18:21:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266992_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 266992_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:02.64 +24:17:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267010_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267010_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:47:43.13 +25:21:30.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 267055_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267055_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:53.43 +16:57:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267079_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267079_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:58:29.93 +22:58:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267081_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267081_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:39:19.74 +24:30:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267116_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267116_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:19:40.18 +24:55:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267121_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267121_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:47:12.35 +18:32:03.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 267184_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267184_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:18.33 +20:20:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267200_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267200_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267256_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267256_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:54:10.85 +19:20:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267280_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267280_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:43:16.63 +23:17:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267283_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267283_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:47:43.31 +17:52:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267335_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267335_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:52:35.74 +19:06:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267362_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267362_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267366_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267366_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267368_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267368_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267371_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267371_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267389_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267389_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:05.72 +23:29:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267419_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267419_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267434_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267434_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267438_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267438_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267479_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267479_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:52:20.89 +17:48:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267481_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267481_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:00:32.95 +23:27:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267510_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267510_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267517_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267517_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:50:59.12 +17:18:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267552_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267552_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267571_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267571_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267572_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267572_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267585_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267585_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:03.65 +24:46:44.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 267654_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267654_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:50:21.45 +24:09:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267681_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267681_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:26.89 +17:56:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267682_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267682_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:26.31 +19:20:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267757_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267757_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267765_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267765_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:58.43 +18:14:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267788_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267788_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267805_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267805_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:47:30.80 +18:20:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267810_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267810_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:47.36 +25:10:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267873_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267873_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:53.78 +26:45:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267912_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267912_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 267924_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267924_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:57.08 +25:08:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267935_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267935_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 267969_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267969_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:52:41.24 +19:43:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267977_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 267977_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:47.06 +24:07:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268028_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268028_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268051_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268051_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:19.66 +26:58:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268072_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268072_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268120_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268120_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:56:03.00 +24:55:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268144_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268144_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268151_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268151_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:03:48.94 +19:29:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268197_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268197_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:41.01 +21:25:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268247_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268247_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:51.53 +18:34:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268255_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268255_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268261_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268261_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:01.21 +24:59:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268307_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268307_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:43:03.88 +24:34:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268329_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268329_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:56:04.52 +25:55:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:43:45.38 +19:58:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268368_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 268368_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 268375_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268375_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:23.53 +22:52:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268379_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268379_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268400_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268400_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:11.95 +22:16:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268457_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268457_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268477_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268477_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:49:21.84 +22:37:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268507_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268507_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:47:59.29 +22:13:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268526_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268526_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:11.50 +21:18:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268548_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268548_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:09.26 +16:55:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268582_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268582_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:32:50.58 +21:17:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268618_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268618_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:50:08.41 +22:32:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268629_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268629_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268632_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268632_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:51.42 +23:08:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268652_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268652_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:06:18.16 +25:34:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268671_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 268671_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 268674_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268674_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268688_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268688_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:25.46 +19:11:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268704_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 268704_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 268727_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268727_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268732_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268732_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268805_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268805_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268813_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268813_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:40:43.74 +22:26:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268846_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268846_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:04.01 +25:35:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268870_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268870_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268889_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268889_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 268902_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268902_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:16.96 +26:19:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268910_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268910_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:39.58 +19:25:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268911_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268911_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:25:59.58 +19:42:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268912_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268912_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:11.99 +18:08:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268920_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268920_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:02:33.59 +17:24:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268970_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268970_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:59.25 +21:59:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268996_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 268996_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:50:51.76 +19:24:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269032_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269032_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:57:26.39 +23:10:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269056_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269056_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:38:21.61 +26:55:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269078_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269078_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:56:45.54 +25:22:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269086_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269086_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:19:49.71 +20:32:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269093_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269093_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 269095_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269095_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:54.69 +22:33:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269101_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269101_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:12:37.47 +19:54:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269112_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269112_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:37:02.74 +26:42:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269113_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269113_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:30.92 +20:25:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269121_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269121_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 269125_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269125_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 269130_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269130_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:55:18.35 +21:26:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269164_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269164_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 269179_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269179_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:30:14.92 +24:10:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:27.52 +22:19:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269202_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269202_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:22.65 +26:05:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269209_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 269209_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 269225_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269225_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:01.92 +20:17:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269233_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 269233_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 269234_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269234_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:37.05 +25:13:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269247_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269247_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:18:43.35 +17:10:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269249_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 269249_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 269262_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269262_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:38.12 +21:45:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269274_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269274_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:20:04.81 +26:11:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269293_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 269293_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 269294_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269294_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:15.95 +17:19:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269314_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269314_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:25:23.73 +17:45:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269317_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269317_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 269332_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269332_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:32:07.15 +26:28:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269333_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269333_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:34:34.66 +24:10:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269335_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269335_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:57.41 +19:48:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269342_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269342_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:37.47 +19:18:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269355_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269355_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 269356_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269356_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:41.97 +25:27:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.296 2023773097949231232 288.42446499643 +25.46463039093 12.7047 11.2108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269358_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269358_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:37:20.90 +20:21:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269359_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269359_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:56.69 +18:22:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.437 4515252251602118912 288.98634801431 +18.37068212666 13.0075 11.5211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269361_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269361_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:01.28 +18:37:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269366_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269366_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:05.14 +17:17:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.721 4513428097416139008 289.27190334814 +17.28994352072 12.8205 11.2817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269386_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269386_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:53:12.37 +17:56:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269393_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269393_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:48.83 +25:44:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269395_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269395_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:36.66 +19:23:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 0.772 4516203127333809152 288.65275146889 +19.39304776150 13.3071 11.8926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269400_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269400_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:37.87 +20:54:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269410_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269410_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:46.67 +24:02:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269412_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269412_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:20:12.67 +20:38:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.911 4516765630597039488 290.05306124146 +20.64443628304 13.0653 11.5587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269417_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269417_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:39:54.86 +25:51:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269430_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269430_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:33.67 +26:39:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.947 2036251966496790400 288.63982556319 +26.66387126968 12.9775 11.4547 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269433_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269433_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:44:04.22 +21:05:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269442_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269442_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:18.80 +23:25:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.919 2022485157523139712 288.82822964365 +23.42058006010 13.1732 11.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269467_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 269467_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:04.87 +19:41:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.099 4515818603170205952 290.52060491171 +19.69558640913 13.0159 11.4881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 164200_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 164200_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:06:08.40 +24:21:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN= 8.99, MAG_FAINT_SEARCH_LIMIT=9.97)GAIADR2_OUTPUT=# 2.518 4533612347750875264 286.53468376740 +24.35427611738 7.8933 6.4666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 127547_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 127547_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:31.15 +22:55:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168667_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 168667_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:31:18.38 +24:41:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153266_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 153266_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 92210_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 92210_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:11.28 +21:02:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93066_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 93066_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:51.52 +21:10:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85058_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 85058_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:21.33 +20:49:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69548_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 69548_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:11:39.76 +20:03:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186482_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 186482_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:35:23.81 +25:45:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184185_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 184185_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:39.56 +25:56:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149186_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 149186_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 109211_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 109211_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:54.73 +22:00:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41462_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 41462_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 164389_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 164389_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 145325_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 145325_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 102257_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 102257_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 218946_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 218946_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 116241_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 116241_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 41009_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 41009_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:17.63 +18:45:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144780_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 144780_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:50:36.59 +23:26:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73122_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 73122_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:58:30.29 +20:06:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98915_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 98915_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 105560_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 105560_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 79257_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 79257_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:06.20 +20:31:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.662 4516865613118143616 289.27564707947 +20.51671929251 12.7535 11.2501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 147392_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 147392_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 123196_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 123196_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 195784_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 195784_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 146284_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 146284_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 109651_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 109651_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:52:31.68 +21:50:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46888_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 46888_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:10:03.40 +18:59:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132414_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 132414_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:00.90 +23:06:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149003_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 149003_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:20:26.89 +23:50:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157126_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 157126_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 59895_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 59895_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 165249_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 165249_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:34:40.33 +24:33:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128837_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 128837_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 163041_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 163041_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 145831_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 145831_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 158551_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 158551_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 170070_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 170070_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 211521_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 211521_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 109555_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 109555_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:17.41 +21:57:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 0.791 4520710296042220928 286.07233916255 +21.95844730497 12.5061 11.0119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101931_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 101931_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 154297_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 154297_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:00.10 +24:02:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157687_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 157687_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 198461_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 198461_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 63878_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 63878_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 64090_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 64090_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 213838_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 213838_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 120042_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 120042_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 111488_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 111488_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:56.99 +22:04:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98790_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 98790_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 84508_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 84508_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:11.08 +20:45:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24232_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 24232_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 136895_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 136895_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 197504_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 197504_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 120448_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 120448_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:49:32.29 +22:27:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157212_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 157212_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 177454_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 177454_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 112620_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 112620_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:12:57.74 +22:08:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245972_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 245972_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 111187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 111187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:32.66 +22:04:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246779_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 246779_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 248324_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 248324_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:53:46.91 +17:16:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176735_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 176735_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:19:04.19 +25:00:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220212_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 220212_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:48.68 +26:27:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155698_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 155698_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:20.43 +24:06:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169835_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 169835_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 126085_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 126085_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 157914_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 157914_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 65768_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 65768_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:28:48.95 +19:53:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103248_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 103248_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:30:44.36 +21:43:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137035_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 137035_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:26:26.37 +23:20:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155717_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 155717_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:12:53.66 +24:07:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04639_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 04639_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 178396_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 178396_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 128239_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 128239_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:10.27 +22:56:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15459_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 15459_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 160837_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 160837_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:37:37.30 +24:20:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134567_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 134567_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 167142_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 167142_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 35606_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 35606_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:33:08.08 +18:29:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186298_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 186298_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:55:26.36 +25:38:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210497_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 210497_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 61064_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 61064_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 120169_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 120169_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:27:58.60 +22:33:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205670_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 205670_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:29.77 +27:03:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68402_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 68402_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:27:16.51 +20:00:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87485_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 87485_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 66993_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 66993_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:03:08.49 +19:52:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42393_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 42393_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 170310_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 170310_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 100996_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 100996_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 173250_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 173250_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:05.91 +24:53:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75603_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 75603_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 146496_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 146496_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:36:32.29 +23:42:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120589_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 120589_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:13.85 +22:27:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30023_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 30023_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 122749_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 122749_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:36.74 +22:39:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 4.790 4520397145714754816 288.65329731066 +22.66103799297 11.3138 9.8272 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208069_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 208069_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:11:03.97 +26:56:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71132_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 71132_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 148523_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 148523_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 178519_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 178519_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 63969_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 63969_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 82363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 82363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:56.16 +20:38:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170408_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 170408_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 134402_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 134402_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:12:42.72 +23:11:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155747_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 155747_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 99402_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 99402_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 162553_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 162553_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 121903_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 121903_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:30:02.75 +22:38:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84346_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 84346_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:14.07 +20:44:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96070_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 96070_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 147080_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 147080_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 194587_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 194587_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 257349_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 257349_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:27.17 +18:38:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72819_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 72819_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:57:30.12 +20:05:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104582_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 104582_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 39127_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 39127_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 256702_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 256702_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:03.06 +19:21:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45834_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 45834_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 142863_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 142863_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 65791_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 65791_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 140617_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 140617_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 63788_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 63788_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:48.53 +19:48:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223165_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 223165_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 254908_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 254908_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (42.2") between the two second-epoch detections
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Considering the candidate 128846_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 128846_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 57875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 57875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 80363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 80363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 221541_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 221541_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 254246_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 254246_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:33:59.57 +20:49:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254179_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 254179_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:59.43 +22:55:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.349 2022405988383477632 288.99760887034 +22.93323556137 12.3359 10.7732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254168_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 254168_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:18:30.75 +22:38:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253954_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 253954_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:44.97 +18:26:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253923_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 253923_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:11:00.06 +17:36:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52717_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 52717_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 50983_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 50983_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 60857_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 60857_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:31:24.82 +19:40:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198053_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 198053_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:55.90 +25:10:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35663_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 35663_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 43344_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 43344_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 29534_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 29534_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:57.26 +18:13:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95295_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 95295_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 161782_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 161782_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 182214_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 182214_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 131200_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 131200_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:55.60 +22:59:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252356_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 252356_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:14.12 +18:44:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74426_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 74426_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:39.34 +20:15:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194552_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 194552_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 85076_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 85076_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:00.83 +20:48:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110438_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 110438_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:53:58.90 +21:54:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63673_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 63673_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:58.20 +19:46:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74353_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 74353_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:17.26 +20:16:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251193_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 251193_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:03:21.38 +24:24:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251168_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 251168_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:10:13.55 +23:20:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113124_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 113124_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 250776_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 250776_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:31:17.80 +18:50:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.396 4323370636284706688 292.82454573024 +18.83500813794 12.2398 10.6615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 10248_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 10248_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:39:21.83 +17:13:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135721_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 135721_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 66716_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 66716_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:09.17 +19:53:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103832_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 103832_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:32:02.80 +21:43:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45243_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 45243_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 45477_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 45477_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:27:22.34 +18:57:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156929_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 156929_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:55.75 +24:11:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121596_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 121596_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 26246_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 26246_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:52:49.44 +17:53:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105577_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 105577_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 48434_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 48434_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 161804_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 161804_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:27:44.12 +24:23:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62627_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 62627_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 70468_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 70468_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:08:15.00 +20:04:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93506_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 93506_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:18:39.23 +21:12:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68192_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 68192_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:12:02.39 +19:58:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 248187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:41:38.22 +18:34:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52097_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 52097_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 113631_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 113631_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 136790_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 136790_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:54:57.49 +23:08:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94797_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 94797_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:38:14.21 +21:15:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 247875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:56:04.05 +17:09:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 172835_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 172835_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:28:50.11 +24:52:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12743_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 12743_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:18:00.31 +17:23:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29456_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 29456_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:26:17.00 +18:12:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82622_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 82622_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:03:29.32 +20:36:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247555_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 247555_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 77535_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 77535_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 246939_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 246939_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 99021_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 99021_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 04891_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 04891_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 72401_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 72401_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 246685_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 246685_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:59.19 +17:32:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246621_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 246621_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:38.15 +17:18:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246236_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 246236_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 246156_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 246156_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 245795_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 245795_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:54.08 +22:52:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.036 2022219419318805504 289.22531837125 +22.88181542467 12.2331 10.7055 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245612_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 245612_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:36:53.12 +19:50:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.796 1825542249672070528 294.22051100548 +19.83921639797 12.2474 10.6198 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245465_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 245465_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 245428_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 245428_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 245420_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 245420_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:00:52.27 +24:39:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 5.223 4533767516327064960 285.21735474646 +24.65166007082 12.8224 11.4423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 127528_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 127528_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 144845_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 144845_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 35648_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 35648_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:44.79 +18:26:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176780_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 176780_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 120885_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 120885_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:32.37 +22:30:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244534_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 244534_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 188748_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 188748_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:36.15 +25:40:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145549_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 145549_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 199891_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 199891_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:32:50.67 +25:13:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243744_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 243744_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:58.20 +20:32:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99815_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 99815_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:30.27 +21:25:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152716_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 152716_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:27.00 +23:58:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160700_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 160700_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 243352_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 243352_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 67760_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 67760_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:36.83 +19:55:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243127_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 243127_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:44.41 +20:46:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.281 4519749464641036544 286.18501069761 +20.77878428758 12.7232 11.1994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243039_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 243039_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:56.72 +23:25:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.925 2022496702396046080 288.73712506690 +23.42194154856 12.8434 11.3410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178056_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 178056_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 182111_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 182111_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:18:33.52 +25:59:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242696_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 242696_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:53.59 +22:38:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.346 4521141858670250496 286.47261401809 +22.64549312295 13.4548 12.0636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134857_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 134857_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 59885_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 59885_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:00:22.71 +19:31:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46951_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 46951_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 228086_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 228086_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:47:57.72 +26:00:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116355_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 116355_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (43.9") between the two second-epoch detections
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Considering the candidate 39971_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 39971_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:26.37 +18:41:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124568_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 124568_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 93916_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 93916_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:08:10.18 +21:11:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59760_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 59760_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:11:17.94 +19:35:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147964_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 147964_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:26:47.20 +23:48:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214809_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 214809_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:39.79 +26:34:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 172826_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 172826_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:27:21.68 +24:52:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87495_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 87495_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 24206_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 24206_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:32:05.95 +17:57:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31561_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 31561_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:49:53.03 +18:13:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181816_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 181816_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 08208_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 08208_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:18.49 +17:07:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19262_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 19262_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:20:44.08 +17:42:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80137_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 80137_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 192745_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 192745_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:33:42.46 +25:30:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07590_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 07590_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 85504_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 85504_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:13.58 +20:48:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197121_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 197121_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 96662_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 96662_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:30.26 +21:22:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152909_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 152909_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 178883_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 178883_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 64408_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 64408_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 131086_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 131086_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 71845_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 71845_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 230445_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 230445_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 196528_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 196528_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 123522_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 123522_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:20.61 +22:40:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230845_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 230845_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 34193_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 34193_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 52709_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 52709_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:53:17.49 +19:07:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 176187_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:21.34 +24:57:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58924_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 58924_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:49.55 +19:34:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79886_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 79886_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 43981_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 43981_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:56.91 +18:52:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159451_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 159451_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 67340_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 67340_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:37.11 +19:58:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174256_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 174256_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:11.56 +24:53:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70659_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 70659_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:41.81 +20:07:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63572_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 63572_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:18:13.69 +19:47:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106400_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 106400_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 71933_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 71933_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:10:31.05 +20:08:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111293_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 111293_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 58390_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 58390_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:16.07 +19:32:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195502_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 195502_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:00:55.47 +25:17:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71275_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 71275_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:11:29.87 +20:05:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141384_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 141384_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:25:54.45 +23:30:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126692_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 126692_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 115901_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 115901_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:23.25 +22:17:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55911_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 55911_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:24.47 +19:25:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43736_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 43736_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:20:13.77 +18:53:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116262_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 116262_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 150156_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 150156_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 29384_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 29384_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 96768_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 96768_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:38.81 +21:20:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128169_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 128169_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:51:10.99 +22:48:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194645_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 194645_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 155957_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 155957_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:03.20 +24:06:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80642_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 80642_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:57:18.72 +20:27:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83356_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 83356_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:22.50 +20:40:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121278_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 121278_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 106739_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 106739_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:19:53.52 +21:53:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24190_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 24190_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 109468_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 109468_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 130143_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 130143_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:04.10 +23:01:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 169875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 195091_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 195091_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 73748_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 73748_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 138844_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 138844_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:21.57 +23:23:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.890 2022495667287340800 288.59025225217 +23.39755132353 11.4752 9.8747 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 11437_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 11437_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:56:52.24 +17:12:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228470_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 228470_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 102969_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 102969_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:20.24 +21:39:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118432_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 118432_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 186960_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 186960_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 90502_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 90502_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 58245_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 58245_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 106960_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 106960_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 168352_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 168352_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 100787_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 100787_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:24.49 +21:33:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16280_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 16280_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:58.55 +17:30:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148167_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 148167_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:28:04.83 +23:48:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95134_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 95134_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 56429_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 56429_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 224669_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 224669_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:56:33.65 +26:05:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67128_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 67128_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 115521_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 115521_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:25:27.05 +22:19:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77024_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 77024_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:09.74 +20:22:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112271_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 112271_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:54.74 +22:08:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188862_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 188862_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 99297_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 99297_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:25:51.36 +21:29:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176389_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 176389_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 176464_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 176464_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:30:20.61 +25:00:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187543_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 187543_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:39.68 +25:39:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32945_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 32945_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 229090_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 229090_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 173606_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 173606_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 49005_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 49005_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 166176_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 166176_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 106158_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 106158_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:23:12.74 +21:52:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.591 2019058731374735104 290.80323516935 +21.87425207298 12.1837 10.6237 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 64112_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 64112_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 230760_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 230760_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:11.83 +26:00:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60469_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 60469_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:32.17 +19:39:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93567_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 93567_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:32:47.30 +21:12:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218205_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 218205_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 74654_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 74654_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 50788_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 50788_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:52:18.37 +19:01:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165592_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 165592_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:27:51.35 +24:34:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167879_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 167879_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:37:41.33 +24:37:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48020_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 48020_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:25:24.58 +19:04:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176350_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 176350_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:34:12.67 +24:59:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111124_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 111124_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:17.70 +22:03:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198581_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 198581_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:05.72 +25:16:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156042_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 156042_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 183687_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 183687_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:47:26.74 +25:48:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177773_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 177773_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 94767_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 94767_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:18.95 +21:17:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197318_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 197318_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:19.79 +25:20:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152784_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 152784_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:30:17.93 +24:00:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55866_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 55866_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 77479_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 77479_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:12:52.49 +20:24:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95665_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 95665_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:33.60 +21:15:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158790_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 158790_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 142697_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 142697_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:14:12.52 +23:33:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183088_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 183088_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 90681_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 90681_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 47630_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 47630_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 193885_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 193885_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 22838_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 22838_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 62884_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 62884_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:39:33.47 +19:43:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 225681_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 225681_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 175636_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 175636_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 04610_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 04610_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:18:59.03 +16:58:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99300_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 99300_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 222956_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 222956_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:19:54.45 +26:20:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226817_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 226817_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 49275_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 49275_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:37.90 +19:04:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184559_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 184559_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 158236_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 158236_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:20:57.46 +24:15:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162016_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 162016_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 39778_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 39778_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:41.17 +18:42:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156873_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 156873_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 176022_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 176022_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 120831_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 120831_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 67963_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 67963_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 197898_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 197898_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:36:52.82 +25:19:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124319_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 124319_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:14.04 +22:44:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113311_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 113311_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:49:59.46 +21:59:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37802_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 37802_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (42.7") between the two second-epoch detections
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Considering the candidate 122847_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 122847_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:56:03.91 +22:31:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128428_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 128428_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:45:37.72 +22:51:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92640_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 92640_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:28:55.13 +21:11:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45618_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 45618_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:11:30.26 +18:56:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229265_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 229265_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 94425_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 94425_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 41604_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 41604_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 65177_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 65177_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:52.07 +19:51:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144507_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 144507_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:31:10.37 +23:30:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157528_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 157528_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:51:34.03 +24:00:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160505_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 160505_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 215782_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 215782_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 95468_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 95468_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:20:26.12 +21:20:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 225789_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 225789_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 66462_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 66462_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:42:39.76 +19:52:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93350_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 93350_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 88231_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 88231_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 48484_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 48484_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 195376_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 195376_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:02.43 +25:23:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28337_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 28337_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 37580_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 37580_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 51985_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 51985_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 224013_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 224013_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:26:44.08 +26:20:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80663_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 80663_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:01.31 +20:31:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47704_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 47704_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:20.65 +19:01:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74819_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 74819_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:41:13.93 +20:15:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13491_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 13491_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 141936_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 141936_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 142878_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 142878_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:57:37.03 +23:26:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117778_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 117778_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 171167_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 171167_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:37:02.36 +24:45:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194266_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 194266_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 157219_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 157219_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 42816_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 42816_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 133561_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 133561_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 176536_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 176536_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:19:51.56 +25:01:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51033_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 51033_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:44.66 +19:11:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195610_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 195610_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 196474_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 196474_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:06:13.34 +25:18:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22912_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 22912_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:54.58 +17:53:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28135_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 28135_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:00.96 +18:02:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30786_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 30786_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 26519_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 26519_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:11.75 +18:01:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 153875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 98515_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 98515_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:38:24.41 +21:23:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136205_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 136205_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:28:07.33 +23:17:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171446_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 171446_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 115780_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 115780_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:16:07.60 +22:19:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115532_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 115532_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:32:52.92 +22:16:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66808_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 66808_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:33.11 +19:56:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65670_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 65670_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:50:59.15 +19:47:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143129_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 143129_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:24:21.26 +23:36:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136573_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 136573_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 137289_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 137289_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:28:32.53 +23:20:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112800_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 112800_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 84113_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 84113_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:11:10.09 +20:44:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.634 4519559141734039552 287.79306938563 +20.73703066769 13.0200 11.5251 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133525_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 133525_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:29:46.92 +23:09:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108131_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 108131_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 131267_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 131267_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:55.11 +23:00:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47326_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 47326_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 207054_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 207054_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:12.75 +26:54:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173273_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 173273_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 161226_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 161226_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 52390_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 52390_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 227017_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 227017_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 213047_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 213047_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 177861_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 177861_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:06:01.41 +25:00:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41190_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 41190_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 74066_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 74066_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 173452_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 173452_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 214916_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 214916_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 163242_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 163242_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 184385_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 184385_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:55:20.34 +25:41:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73391_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 73391_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 72488_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 72488_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:55.72 +20:12:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56531_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 56531_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 76526_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 76526_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:54.05 +20:17:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83833_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 83833_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 90410_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 90410_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:00:39.20 +20:56:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71668_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 71668_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:13:15.02 +20:05:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127802_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 127802_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 112118_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 112118_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 125235_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 125235_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 66100_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 66100_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 70708_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 70708_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 117196_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 117196_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 171683_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 171683_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:08:30.02 +24:42:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127370_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 127370_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 78513_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 78513_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:11:28.52 +20:27:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137042_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 137042_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:28.10 +23:09:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43085_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 43085_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 102200_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 102200_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 185247_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 185247_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:27.10 +25:51:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 3.319 2023980111058771712 290.36338346499 +25.86176518553 12.7030 11.2573 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 121633_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 121633_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:50:42.50 +22:29:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67974_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 67974_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 119593_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 119593_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 77066_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 77066_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:01:34.73 +20:18:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170404_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 170404_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 173597_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 173597_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 59733_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 59733_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:02:41.64 +19:32:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27901_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 27901_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:58:58.00 +18:00:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99126_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 99126_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:03:48.37 +21:23:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22248_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 22248_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:14.79 +17:45:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223916_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 223916_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:48.17 +26:18:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223399_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 223399_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:03:19.51 +26:13:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158509_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 158509_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:26:46.10 +24:16:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199317_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 199317_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:59:58.99 +25:07:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63165_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 63165_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:12:53.76 +19:44:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26936_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 26936_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 119878_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 119878_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:55:56.79 +22:20:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14231_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 14231_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:31.55 +17:21:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74700_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 74700_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 229776_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 229776_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 77690_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 77690_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 130275_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 130275_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:15:54.27 +22:59:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124668_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 124668_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 136229_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 136229_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 216093_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 216093_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 211544_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 211544_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 85752_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 85752_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:04:07.48 +20:46:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113819_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 113819_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 49820_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 49820_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 111592_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 111592_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:11:00.69 +21:59:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70523_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 70523_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:06:17.94 +19:59:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153788_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 153788_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 40947_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 40947_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:07:52.31 +18:43:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26361_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 26361_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:33:24.01 +18:01:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123162_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 123162_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:03:43.33 +22:37:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129982_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 129982_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:05:49.12 +22:57:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.789 4521343790849093248 286.45417001838 +22.95927751873 12.7893 11.3805 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214399_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 214399_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 225882_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 225882_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 226933_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 226933_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:25:24.87 +26:10:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27738_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 27738_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:56.25 +18:00:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47896_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 47896_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:17:55.43 +19:03:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127706_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 127706_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 38352_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 38352_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:37.52 +18:35:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178847_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 178847_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:27:06.11 +25:06:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152346_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 152346_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 113523_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 113523_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:52:53.80 +22:00:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62403_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 62403_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:01.17 +19:44:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198339_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 198339_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 81363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 81363_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:01:04.71 +20:31:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47024_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 47024_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:22:47.54 +19:01:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57504_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 57504_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 96095_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 96095_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 43771_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 43771_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 169142_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 169142_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:21:44.33 +24:43:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39304_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 39304_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 224683_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 224683_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 19762_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 19762_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 104245_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 104245_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:52:40.58 +21:34:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80794_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 80794_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 15326_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 15326_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 88891_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 88891_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 27749_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 27749_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 118717_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 118717_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 51955_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 51955_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 95404_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 95404_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 78116_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 78116_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 90362_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 90362_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:31:38.23 +21:04:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66061_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 66061_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:36:19.74 +19:53:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118391_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 118391_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 90353_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 90353_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:09:59.89 +21:02:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114959_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 114959_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:03:49.07 +22:12:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114831_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 114831_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 142823_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 142823_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:40:20.10 +23:32:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160459_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 160459_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 96987_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 96987_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 162808_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 162808_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 14755_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 14755_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:28:32.69 +17:29:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76647_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 76647_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 52707_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 52707_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 148355_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 148355_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:33:17.74 +23:39:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121996_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 121996_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:20:40.59 +22:38:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127908_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 127908_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
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Considering the candidate 79875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 79875_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 74450_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
Preparing report for the candidate 74450_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
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Considering the candidate 19372_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 19372_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 19:08:45.18 +17:41:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128454_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005
The candidate 128454_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005 did not pass the final checks
**** FOUND 18:54:45.06 +22:38:45.0 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 19s
make_report_in_HTML.sh TOTAL: 736s
Prepared the HTML report for the field Vul-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:18:46.36 +16:59:32.5
19:19:56.96 +17:07:46.7
18:59:52.04 +21:30:00.8
19:32:51.16 +21:39:03.9
18:54:10.89 +21:29:23.6
19:35:36.39 +21:46:10.2
19:01:48.83 +21:46:54.5
19:26:27.15 +21:54:37.6
19:24:49.77 +21:56:45.4
18:51:56.48 +21:48:11.3
19:09:13.19 +22:04:03.1
18:56:24.44 +22:00:30.1
19:28:32.61 +22:12:07.1
19:16:46.42 +22:16:41.1
19:27:18.11 +22:21:35.6
19:04:37.40 +22:16:09.2
19:14:22.83 +22:22:29.7
19:23:42.39 +22:27:26.1
19:05:07.40 +22:24:35.3
19:08:11.28 +22:28:15.7
19:17:59.97 +22:31:43.0
19:14:01.25 +22:32:19.9
18:55:25.62 +22:25:43.9
18:58:55.16 +22:29:54.0
19:23:06.05 +22:46:36.3
19:09:56.06 +22:44:17.5
19:24:22.28 +22:48:54.0
18:55:46.19 +22:42:45.2
19:02:38.51 +22:49:16.6
19:05:16.09 +22:51:13.2
19:15:03.21 +22:56:16.0
19:31:50.37 +22:57:36.8
19:11:15.58 +23:01:23.0
19:13:46.16 +23:09:28.1
19:21:40.69 +23:13:37.9
18:53:02.65 +23:01:35.7
19:35:19.57 +17:24:41.7
19:12:41.16 +23:14:43.6
19:06:44.52 +23:13:33.0
19:14:52.38 +23:17:46.6
19:15:27.13 +23:28:48.0
18:57:41.63 +23:24:27.7
19:21:48.73 +23:35:18.9
19:26:54.27 +23:40:26.7
19:15:54.02 +23:41:30.6
19:24:05.92 +23:43:30.8
19:09:13.44 +23:42:57.0
19:13:42.11 +23:43:58.1
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19:17:59.22 +17:31:47.2
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19:26:41.80 +24:12:26.7
19:08:01.85 +24:09:34.7
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19:10:00.84 +24:22:08.4
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19:11:46.21 +24:43:52.8
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19:16:11.78 +25:02:27.7
19:21:38.56 +25:05:04.8
19:23:27.89 +25:05:34.3
19:40:36.73 +25:02:46.0
19:04:34.08 +25:57:43.4
19:11:21.37 +25:55:53.5
19:42:53.52 +25:50:57.5
19:20:26.46 +25:52:12.4
19:10:28.53 +25:43:55.9
19:11:28.80 +25:39:16.6
18:59:33.41 +25:19:57.2
19:07:08.69 +25:24:15.4
19:02:51.26 +25:24:55.2
19:36:46.07 +25:24:56.3
19:01:04.19 +25:18:27.2
19:04:12.03 +25:17:58.8
19:21:02.45 +25:23:42.5
19:17:29.24 +25:21:17.2
19:36:37.67 +25:17:22.4
19:22:11.80 +17:44:10.2
19:16:30.20 +25:16:30.4
19:04:40.56 +26:45:09.9
19:45:50.07 +26:44:26.9
19:48:11.32 +26:43:32.3
19:12:05.80 +26:43:15.3
19:16:00.88 +26:44:19.9
19:04:45.78 +26:35:53.3
19:30:53.51 +26:39:50.1
19:13:41.77 +26:37:44.3
19:39:20.36 +26:34:31.1
19:24:05.81 +26:32:44.3
19:21:09.98 +26:31:01.9
19:13:34.95 +26:22:44.8
19:39:21.13 +26:18:43.7
19:16:20.28 +26:21:24.3
19:41:49.63 +26:10:38.7
19:04:31.95 +26:09:09.7
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19:31:55.92 +26:11:20.9
19:31:11.12 +26:10:51.4
19:11:16.89 +17:51:52.5
19:31:30.63 +26:07:04.2
19:20:35.75 +26:05:56.7
19:03:43.93 +25:59:04.1
19:17:36.52 +26:01:42.1
19:33:34.37 +26:01:17.2
19:16:58.11 +17:56:55.6
19:12:49.22 +17:56:29.7
19:42:36.43 +25:08:47.5
19:55:25.63 +23:27:13.8
19:26:25.48 +22:35:58.4
18:54:24.04 +23:33:16.1
18:58:45.23 +25:27:15.4
19:19:27.87 +24:26:21.3
19:39:17.76 +18:21:34.8
19:52:13.65 +26:35:19.1
19:27:43.61 +26:08:30.5
19:26:16.91 +18:00:18.5
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19:46:47.03 +18:01:59.9
19:01:16.48 +18:03:00.1
19:37:10.15 +18:11:20.3
19:35:38.44 +18:13:38.0
19:17:19.37 +18:22:16.5
19:23:04.43 +18:35:57.1
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19:05:02.23 +18:38:05.2
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19:22:01.80 +19:17:34.6
19:09:14.98 +19:23:11.5
19:11:10.27 +19:26:32.1
19:23:07.44 +19:28:30.4
19:08:35.55 +19:29:07.5
19:12:46.73 +19:31:41.7
18:56:17.36 +19:28:47.5
19:11:29.36 +19:39:17.9
19:13:15.22 +19:43:07.2
19:21:09.97 +19:48:39.8
19:05:23.82 +19:44:23.9
19:31:32.56 +19:49:59.7
19:31:34.02 +19:54:00.4
19:07:35.33 +19:51:27.0
19:13:27.45 +19:56:12.9
19:34:11.94 +19:58:28.2
19:01:55.84 +19:53:52.5
19:20:10.34 +20:06:48.5
19:03:17.58 +20:03:09.5
19:11:08.80 +20:07:04.0
19:09:43.79 +20:09:13.8
19:22:04.22 +20:14:03.6
19:13:06.67 +20:14:10.4
19:22:00.22 +20:16:29.2
19:07:00.45 +20:14:09.9
19:12:14.83 +20:15:55.0
18:50:58.78 +20:11:35.6
18:50:51.69 +20:11:21.2
19:12:40.49 +20:26:28.9
19:24:47.32 +20:32:41.6
19:01:19.68 +20:28:27.5
19:05:42.92 +20:31:51.8
19:18:23.45 +20:44:33.1
19:10:07.59 +20:53:42.5
19:24:43.81 +20:56:00.4
18:51:42.33 +20:47:54.9
18:50:46.51 +20:52:25.8
19:43:53.74 +21:01:40.8
19:20:10.97 +21:17:23.2
19:00:04.96 +21:11:47.5
19:19:51.09 +21:19:39.1
19:12:15.22 +21:20:38.1
19:02:36.44 +21:09:36.7
19:16:56.80 +21:23:28.5
19:13:02.37 +21:28:55.4
18:57:56.52 +21:21:20.1
19:17:02.90 +21:30:04.1
Source monitoring: measuring positions from /data_ssd/NMW-TexasTech/workdir/img_2026-11-03_CI_Vul-01-Q1b1x1_222054_TTUQ1b1x1_2393500_Dy7Ladh9/monitoring_positions.txt
Source monitoring: positions closer than 100 pix to a frame edge are recorded as edge
Read 98277 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 282.2101 to 299.8008 deg, Dec +16.2510 to +27.3920 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 282.2101 to 299.8008 deg, Dec 16.2510 to 27.3920 deg
Loaded 19894 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): 12775 out of 15241 total matches.
Matched with Tycho-2 15241 out of 98277 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
Observation time (mid-exposure, UTC): JD 2461348.68003 (FITS header)
Observing site: lat= +33.748056 deg lon= -101.958333 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 290.77163 deg Dec= +22.00277 deg
Frame center: alt= +23.640 deg az= 279.603 deg airmass= 2.4765
Header cross-check: CENTALT= 23.863 deg (difference -0.222 deg)
Header cross-check: AIRMASS= 2.4597 (we compute 2.4765)
Airmass zero-point fit: OK k= +0.1902 +/- 0.0065 mag/airmass N= 5397 airmass span 1.8338-3.9863 scatter 0.2207 mag
Source monitoring: airmass zero-point for wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits: OK +0.531614 -0.190224 2.4765 +0.1902 5397 2.1526 0.2207 1.8338 3.9863
Edge margin: 100.0 pix (FORCED_PHOTOMETRY_EDGE_MARGIN_PIX)
Forced photometry (list mode): image=wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits list=monitoring_pixlist2403546.tmp aperture=7.3
Image size: 9576 x 6388
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 22.478200
Local star coverage test: 98277 stars in wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits.wcscat, test radius 301 pix (0.50 deg), 464.7 stars per circle at the frame's mean density
Forced photometry: center=(1533.31, 5192.66) aperture=7.3
Annulus: inner=14.60 outer=36.50 edge margin=100.00
Background annulus: 3516 pixels
Iterative clipping converged after 5 iterations, 3318/3516 pixels remain
SExtractor background: mode=1003.88 median=1015.00 mean=1022.41 sigma=75.46 -> bg=1003.88 (3318 pixels)
Aperture sum=54415.40 N_eff=41.8539
Net flux=12398.94 noise=488.21 SNR=25.40
Instrumental magnitude: -10.2335
Calibrated magnitude: 12.2447
Local star coverage at (1533.31, 5192.66): 713 catalog stars within 301 pix, 464.7 expected at the frame's mean star density
Source monitoring: airmass zero-point term applied to the measurements on wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits
Source monitoring: 1 position(s) measured on wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-04_20.00sec_-0.00C_LIGHTs_0004.fits (aperture 7.3 pix)
Read 101929 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 282.1953 to 299.7625 deg, Dec +16.2519 to +27.3981 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 282.1953 to 299.7625 deg, Dec 16.2519 to 27.3981 deg
Loaded 19859 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): 12633 out of 15151 total matches.
Matched with Tycho-2 15151 out of 101929 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
Observation time (mid-exposure, UTC): JD 2461348.68066 (FITS header)
Observing site: lat= +33.748056 deg lon= -101.958333 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 290.76061 deg Dec= +22.00934 deg
Frame center: alt= +23.450 deg az= 279.705 deg airmass= 2.4951
Header cross-check: CENTALT= 23.679 deg (difference -0.229 deg)
Header cross-check: AIRMASS= 2.4774 (we compute 2.4951)
Airmass zero-point fit: OK k= +0.2047 +/- 0.0065 mag/airmass N= 5263 airmass span 1.8450-3.9440 scatter 0.2178 mag
Source monitoring: airmass zero-point for wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits: OK +0.570015 -0.204680 2.4951 +0.2047 5263 2.0989 0.2178 1.8450 3.9440
Edge margin: 100.0 pix (FORCED_PHOTOMETRY_EDGE_MARGIN_PIX)
Forced photometry (list mode): image=wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits list=monitoring_pixlist2403546.tmp aperture=7.2
Image size: 9576 x 6388
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 22.509200
Local star coverage test: 101929 stars in wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits.wcscat, test radius 301 pix (0.50 deg), 482.0 stars per circle at the frame's mean density
Forced photometry: center=(1526.54, 5196.07) aperture=7.2
Annulus: inner=14.40 outer=36.00 edge margin=100.00
Background annulus: 3429 pixels
Iterative clipping converged after 6 iterations, 3238/3429 pixels remain
SExtractor background: mode=1014.40 median=1026.00 mean=1033.73 sigma=74.11 -> bg=1014.40 (3238 pixels)
Aperture sum=53235.34 N_eff=40.7150
Net flux=11933.95 noise=472.90 SNR=25.24
Instrumental magnitude: -10.1920
Calibrated magnitude: 12.3172
Local star coverage at (1526.54, 5196.07): 695 catalog stars within 301 pix, 482.0 expected at the frame's mean star density
Source monitoring: airmass zero-point term applied to the measurements on wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits
Source monitoring: 1 position(s) measured on wcs_fd_Vul-01-Q1b1x1_2026-11-03_22-19-58_20.00sec_-0.00C_LIGHTs_0005.fits (aperture 7.2 pix)
########### Completed Vul-01-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 ####
19:26:25.48 +22:35:58.4
18:54:24.04 +23:33:16.1
18:58:45.23 +25:27:15.4
19:19:27.87 +24:26:21.3
19:39:17.76 +18:21:34.8
19:52:13.65 +26:35:19.1
19:27:43.61 +26:08:30.5
19:26:16.91 +18:00:18.5
19:26:05.19 +17:26:57.3
19:33:24.58 +24:18:23.9
19:21:43.99 +24:02:05.0
19:32:37.28 +23:50:58.9
19:01:00.32 +18:41:45.8
19:21:09.98 +26:31:01.9
19:27:18.11 +22:21:35.6
18:57:56.52 +21:21:20.1
19:13:42.11 +23:43:58.1
19:21:02.45 +25:23:42.5
19:24:05.92 +23:43:30.8
19:26:41.80 +24:12:26.7
18:56:17.36 +19:28:47.5
19:15:03.21 +22:56:16.0
19:10:23.03 +24:24:57.2
19:17:29.53 +24:16:05.4
19:12:01.63 +24:43:11.1
19:45:50.07 +26:44:26.9
19:32:51.16 +21:39:03.9
19:15:37.49 +24:12:07.9
19:16:00.88 +26:44:19.9
19:17:59.97 +22:31:43.0
19:13:02.37 +21:28:55.4
19:12:49.22 +17:56:29.7
19:14:52.38 +23:17:46.6
19:36:37.67 +25:17:22.4
19:23:43.61 +25:03:39.4
19:18:05.50 +24:44:03.7
19:12:48.22 +24:12:51.5
19:23:27.89 +25:05:34.3
19:17:59.22 +17:31:47.2
19:21:40.69 +23:13:37.9
19:12:07.74 +24:36:54.6
19:04:40.56 +26:45:09.9
19:11:29.36 +19:39:17.9
19:10:07.59 +20:53:42.5
19:11:46.21 +24:43:52.8
18:59:52.04 +21:30:00.8
19:35:38.44 +18:13:38.0
19:03:17.58 +20:03:09.5
18:57:38.82 +23:40:46.4
19:21:09.97 +19:48:39.8
19:04:33.28 +24:40:51.8
19:12:15.22 +21:20:38.1
19:09:13.44 +23:42:57.0
19:02:51.26 +25:24:55.2
19:35:36.39 +21:46:10.2
18:50:46.82 +18:29:26.7
19:14:44.03 +18:56:50.2
19:21:48.73 +23:35:18.9
19:31:34.02 +19:54:00.4
19:15:27.13 +23:28:48.0
19:39:21.13 +26:18:43.7
19:31:50.37 +22:57:36.8
19:01:19.68 +20:28:27.5
19:13:34.95 +26:22:44.8
19:10:34.16 +19:11:06.6
19:09:27.26 +18:49:47.5
19:19:51.09 +21:19:39.1
19:20:23.11 +24:24:41.3
19:11:21.37 +25:55:53.5
19:28:32.61 +22:12:07.1
19:12:41.16 +23:14:43.6
18:58:55.16 +22:29:54.0
19:10:39.39 +19:03:48.4
19:13:15.22 +19:43:07.2
19:15:05.14 +19:15:09.2
19:55:25.63 +23:27:13.8
19:18:46.36 +16:59:32.5
19:09:43.79 +20:09:13.8
19:02:38.51 +22:49:16.6
19:26:54.27 +23:40:26.7
19:15:54.02 +23:41:30.6
19:44:53.21 +24:17:36.4
19:42:36.43 +25:08:47.5
19:21:38.56 +25:05:04.8
18:53:02.65 +23:01:35.7
19:10:20.17 +18:59:47.6
19:23:06.05 +22:46:36.3
19:24:43.81 +20:56:00.4
19:04:34.08 +25:57:43.4
19:19:56.96 +17:07:46.7
19:40:34.48 +23:58:08.3
19:40:36.73 +25:02:46.0
19:31:32.56 +19:49:59.7
19:11:15.58 +23:01:23.0
19:11:08.80 +20:07:04.0
19:17:36.52 +26:01:42.1
19:17:29.24 +25:21:17.2
19:33:34.37 +26:01:17.2
19:45:06.35 +18:22:43.0
19:09:27.93 +24:15:29.9
19:01:48.83 +21:46:54.5
19:09:13.19 +22:04:03.1
19:04:37.40 +22:16:09.2
19:06:18.03 +23:50:04.4
19:37:10.15 +18:11:20.3
19:36:46.07 +25:24:56.3
18:55:25.62 +22:25:43.9
19:16:58.11 +17:56:55.6
18:51:56.48 +21:48:11.3
19:38:20.76 +24:43:00.1
19:01:04.19 +25:18:27.2
19:13:06.67 +20:14:10.4
19:31:30.63 +26:07:04.2
19:10:28.53 +25:43:55.9
18:50:46.51 +20:52:25.8
19:12:46.73 +19:31:41.7
19:26:27.15 +21:54:37.6
19:10:45.25 +24:37:51.3
19:00:04.96 +21:11:47.5
19:11:10.27 +19:26:32.1
19:13:27.45 +19:56:12.9
19:11:28.80 +25:39:16.6
19:14:56.57 +24:59:41.7
19:17:19.37 +18:22:16.5
19:05:23.82 +19:44:23.9
19:24:05.81 +26:32:44.3
19:12:14.83 +20:15:55.0
19:22:55.04 +24:09:57.5
19:16:11.78 +25:02:27.7
19:09:14.98 +19:23:11.5
19:25:28.98 +24:17:10.1
19:42:53.52 +25:50:57.5
19:43:53.74 +21:01:40.8
19:07:08.11 +18:59:17.0
18:59:33.41 +25:19:57.2
19:11:16.89 +17:51:52.5
19:41:49.63 +26:10:38.7
19:09:06.61 +24:55:01.5
19:17:02.90 +21:30:04.1
19:31:55.92 +26:11:20.9
19:20:26.46 +25:52:12.4
19:10:00.84 +24:22:08.4
19:21:45.26 +24:11:49.1
19:16:02.54 +24:59:07.1
19:14:01.25 +22:32:19.9
19:34:11.94 +19:58:28.2
19:20:35.75 +26:05:56.7
19:20:10.97 +21:17:23.2
19:20:55.77 +18:47:27.5
19:12:10.30 +24:18:34.4
19:13:41.77 +26:37:44.3
19:04:31.95 +26:09:09.7
19:17:52.50 +19:05:42.0
19:23:04.43 +18:35:57.1
19:14:41.04 +19:15:01.6
19:35:19.57 +17:24:41.7
18:57:41.63 +23:24:27.7
19:07:08.69 +25:24:15.4
19:08:01.85 +24:09:34.7
19:10:15.92 +18:48:39.0
19:13:46.16 +23:09:28.1
19:04:12.03 +25:17:58.8
19:04:13.03 +23:58:52.3
19:31:02.92 +24:48:43.5
18:56:24.44 +22:00:30.1
19:24:49.77 +21:56:45.4
19:30:31.21 +24:53:03.7
19:00:55.84 +24:14:59.4
19:02:35.08 +19:11:56.7
19:31:11.12 +26:10:51.4
19:12:05.80 +26:43:15.3
19:12:07.45 +18:44:50.5
19:22:00.22 +20:16:29.2
19:04:36.17 +24:48:39.8
19:30:53.51 +26:39:50.1
19:23:14.09 +24:27:38.1
19:22:04.22 +20:14:03.6
19:23:07.44 +19:28:30.4
19:18:23.45 +20:44:33.1
19:05:16.09 +22:51:13.2
19:24:22.28 +22:48:54.0
19:07:35.33 +19:51:27.0
19:20:10.34 +20:06:48.5
19:14:22.83 +22:22:29.7
18:55:46.19 +22:42:45.2
19:12:04.80 +18:50:25.1
18:54:10.89 +21:29:23.6
19:01:55.84 +19:53:52.5
19:08:11.28 +22:28:15.7
19:15:27.07 +24:45:21.9
19:00:27.72 +24:43:46.3
19:46:47.03 +18:01:59.9
19:03:43.93 +25:59:04.1
18:50:51.69 +20:11:21.2
19:09:56.06 +22:44:17.5
19:06:44.52 +23:13:33.0
19:39:20.36 +26:34:31.1
19:48:11.32 +26:43:32.3
19:20:38.86 +19:09:45.6
19:09:45.51 +24:01:34.9
19:04:45.78 +26:35:53.3
19:09:59.05 +26:11:25.6
19:24:07.20 +23:59:24.5
19:16:30.20 +25:16:30.4
19:08:35.55 +19:29:07.5
19:02:36.44 +21:09:36.7
19:13:43.42 +18:52:08.2
19:05:02.23 +18:38:05.2
19:16:20.28 +26:21:24.3
19:22:11.80 +17:44:10.2
19:05:42.92 +20:31:51.8
18:51:42.33 +20:47:54.9
19:01:16.48 +18:03:00.1
19:05:07.40 +22:24:35.3
19:12:40.49 +20:26:28.9
19:23:42.39 +22:27:26.1
19:16:46.42 +22:16:41.1
19:16:56.80 +21:23:28.5
18:50:58.78 +20:11:35.6
19:22:01.80 +19:17:34.6
19:24:47.32 +20:32:41.6
19:07:00.45 +20:14:09.9
###################################################################################
19:26:25.48 +22:35:58.4 -- not an asteroid (will add it to exclusion list)
18:54:24.04 +23:33:16.1 -- not an asteroid (will add it to exclusion list)
18:58:45.23 +25:27:15.4 -- not an asteroid (will add it to exclusion list)
19:19:27.87 +24:26:21.3 -- not an asteroid (will add it to exclusion list)
19:39:17.76 +18:21:34.8 -- not an asteroid (will add it to exclusion list)
19:52:13.65 +26:35:19.1 -- not an asteroid (will add it to exclusion list)
19:27:43.61 +26:08:30.5 -- not an asteroid (will add it to exclusion list)
19:26:16.91 +18:00:18.5 -- not an asteroid (will add it to exclusion list)
19:26:05.19 +17:26:57.3 -- not an asteroid (will add it to exclusion list)
19:33:24.58 +24:18:23.9 -- not an asteroid (will add it to exclusion list)
19:21:43.99 +24:02:05.0 -- not an asteroid (will add it to exclusion list)
19:32:37.28 +23:50:58.9 -- not an asteroid (will add it to exclusion list)
19:01:00.32 +18:41:45.8 -- not an asteroid (will add it to exclusion list)
19:21:09.98 +26:31:01.9 -- not an asteroid (will add it to exclusion list)
19:27:18.11 +22:21:35.6 -- not an asteroid (will add it to exclusion list)
18:57:56.52 +21:21:20.1 -- not an asteroid (will add it to exclusion list)
19:13:42.11 +23:43:58.1 -- not an asteroid (will add it to exclusion list)
19:21:02.45 +25:23:42.5 -- not an asteroid (will add it to exclusion list)
19:24:05.92 +23:43:30.8 -- not an asteroid (will add it to exclusion list)
19:26:41.80 +24:12:26.7 -- not an asteroid (will add it to exclusion list)
18:56:17.36 +19:28:47.5 -- not an asteroid (will add it to exclusion list)
19:15:03.21 +22:56:16.0 -- not an asteroid (will add it to exclusion list)
19:10:23.03 +24:24:57.2 -- not an asteroid (will add it to exclusion list)
19:17:29.53 +24:16:05.4 -- not an asteroid (will add it to exclusion list)
19:12:01.63 +24:43:11.1 -- not an asteroid (will add it to exclusion list)
19:45:50.07 +26:44:26.9 -- not an asteroid (will add it to exclusion list)
19:32:51.16 +21:39:03.9 -- not an asteroid (will add it to exclusion list)
19:15:37.49 +24:12:07.9 -- not an asteroid (will add it to exclusion list)
19:16:00.88 +26:44:19.9 -- not an asteroid (will add it to exclusion list)
19:17:59.97 +22:31:43.0 -- not an asteroid (will add it to exclusion list)
19:13:02.37 +21:28:55.4 -- not an asteroid (will add it to exclusion list)
19:12:49.22 +17:56:29.7 -- not an asteroid (will add it to exclusion list)
19:14:52.38 +23:17:46.6 -- not an asteroid (will add it to exclusion list)
19:36:37.67 +25:17:22.4 -- not an asteroid (will add it to exclusion list)
19:23:43.61 +25:03:39.4 -- not an asteroid (will add it to exclusion list)
19:18:05.50 +24:44:03.7 -- not an asteroid (will add it to exclusion list)
19:12:48.22 +24:12:51.5 -- not an asteroid (will add it to exclusion list)
19:23:27.89 +25:05:34.3 -- not an asteroid (will add it to exclusion list)
19:17:59.22 +17:31:47.2 -- not an asteroid (will add it to exclusion list)
19:21:40.69 +23:13:37.9 -- not an asteroid (will add it to exclusion list)
19:12:07.74 +24:36:54.6 -- not an asteroid (will add it to exclusion list)
19:04:40.56 +26:45:09.9 -- not an asteroid (will add it to exclusion list)
19:11:29.36 +19:39:17.9 -- not an asteroid (will add it to exclusion list)
19:10:07.59 +20:53:42.5 -- not an asteroid (will add it to exclusion list)
19:11:46.21 +24:43:52.8 -- not an asteroid (will add it to exclusion list)
18:59:52.04 +21:30:00.8 -- not an asteroid (will add it to exclusion list)
19:35:38.44 +18:13:38.0 -- not an asteroid (will add it to exclusion list)
19:03:17.58 +20:03:09.5 -- not an asteroid (will add it to exclusion list)
18:57:38.82 +23:40:46.4 -- not an asteroid (will add it to exclusion list)
19:21:09.97 +19:48:39.8 -- not an asteroid (will add it to exclusion list)
19:04:33.28 +24:40:51.8 -- not an asteroid (will add it to exclusion list)
19:12:15.22 +21:20:38.1 -- not an asteroid (will add it to exclusion list)
19:09:13.44 +23:42:57.0 -- not an asteroid (will add it to exclusion list)
19:02:51.26 +25:24:55.2 -- not an asteroid (will add it to exclusion list)
19:35:36.39 +21:46:10.2 -- not an asteroid (will add it to exclusion list)
18:50:46.82 +18:29:26.7 -- not an asteroid (will add it to exclusion list)
19:14:44.03 +18:56:50.2 -- not an asteroid (will add it to exclusion list)
19:21:48.73 +23:35:18.9 -- not an asteroid (will add it to exclusion list)
19:31:34.02 +19:54:00.4 -- not an asteroid (will add it to exclusion list)
19:15:27.13 +23:28:48.0 -- not an asteroid (will add it to exclusion list)
19:39:21.13 +26:18:43.7 -- not an asteroid (will add it to exclusion list)
19:31:50.37 +22:57:36.8 -- not an asteroid (will add it to exclusion list)
19:01:19.68 +20:28:27.5 -- not an asteroid (will add it to exclusion list)
19:13:34.95 +26:22:44.8 -- not an asteroid (will add it to exclusion list)
19:10:34.16 +19:11:06.6 -- not an asteroid (will add it to exclusion list)
19:09:27.26 +18:49:47.5 -- not an asteroid (will add it to exclusion list)
19:19:51.09 +21:19:39.1 -- not an asteroid (will add it to exclusion list)
19:20:23.11 +24:24:41.3 -- not an asteroid (will add it to exclusion list)
19:11:21.37 +25:55:53.5 -- not an asteroid (will add it to exclusion list)
19:28:32.61 +22:12:07.1 -- not an asteroid (will add it to exclusion list)
19:12:41.16 +23:14:43.6 -- not an asteroid (will add it to exclusion list)
18:58:55.16 +22:29:54.0 -- not an asteroid (will add it to exclusion list)
19:10:39.39 +19:03:48.4 -- not an asteroid (will add it to exclusion list)
19:13:15.22 +19:43:07.2 -- not an asteroid (will add it to exclusion list)
19:15:05.14 +19:15:09.2 -- not an asteroid (will add it to exclusion list)
19:55:25.63 +23:27:13.8 -- not an asteroid (will add it to exclusion list)
19:18:46.36 +16:59:32.5 -- not an asteroid (will add it to exclusion list)
19:09:43.79 +20:09:13.8 -- not an asteroid (will add it to exclusion list)
19:02:38.51 +22:49:16.6 -- not an asteroid (will add it to exclusion list)
19:26:54.27 +23:40:26.7 -- not an asteroid (will add it to exclusion list)
19:15:54.02 +23:41:30.6 -- not an asteroid (will add it to exclusion list)
19:44:53.21 +24:17:36.4 -- not an asteroid (will add it to exclusion list)
19:42:36.43 +25:08:47.5 -- not an asteroid (will add it to exclusion list)
19:21:38.56 +25:05:04.8 -- not an asteroid (will add it to exclusion list)
18:53:02.65 +23:01:35.7 -- not an asteroid (will add it to exclusion list)
19:10:20.17 +18:59:47.6 -- not an asteroid (will add it to exclusion list)
19:23:06.05 +22:46:36.3 -- not an asteroid (will add it to exclusion list)
19:24:43.81 +20:56:00.4 -- not an asteroid (will add it to exclusion list)
19:04:34.08 +25:57:43.4 -- not an asteroid (will add it to exclusion list)
19:19:56.96 +17:07:46.7 -- not an asteroid (will add it to exclusion list)
19:40:34.48 +23:58:08.3 -- not an asteroid (will add it to exclusion list)
19:40:36.73 +25:02:46.0 -- not an asteroid (will add it to exclusion list)
19:31:32.56 +19:49:59.7 -- not an asteroid (will add it to exclusion list)
19:11:15.58 +23:01:23.0 -- not an asteroid (will add it to exclusion list)
19:11:08.80 +20:07:04.0 -- not an asteroid (will add it to exclusion list)
19:17:36.52 +26:01:42.1 -- not an asteroid (will add it to exclusion list)
19:17:29.24 +25:21:17.2 -- not an asteroid (will add it to exclusion list)
19:33:34.37 +26:01:17.2 -- not an asteroid (will add it to exclusion list)
19:45:06.35 +18:22:43.0 -- not an asteroid (will add it to exclusion list)
19:09:27.93 +24:15:29.9 -- not an asteroid (will add it to exclusion list)
19:01:48.83 +21:46:54.5 -- not an asteroid (will add it to exclusion list)
19:09:13.19 +22:04:03.1 -- not an asteroid (will add it to exclusion list)
19:04:37.40 +22:16:09.2 -- not an asteroid (will add it to exclusion list)
19:06:18.03 +23:50:04.4 -- not an asteroid (will add it to exclusion list)
19:37:10.15 +18:11:20.3 -- not an asteroid (will add it to exclusion list)
19:36:46.07 +25:24:56.3 -- not an asteroid (will add it to exclusion list)
18:55:25.62 +22:25:43.9 -- not an asteroid (will add it to exclusion list)
19:16:58.11 +17:56:55.6 -- not an asteroid (will add it to exclusion list)
18:51:56.48 +21:48:11.3 -- not an asteroid (will add it to exclusion list)
19:38:20.76 +24:43:00.1 -- not an asteroid (will add it to exclusion list)
19:01:04.19 +25:18:27.2 -- not an asteroid (will add it to exclusion list)
19:13:06.67 +20:14:10.4 -- not an asteroid (will add it to exclusion list)
19:31:30.63 +26:07:04.2 -- not an asteroid (will add it to exclusion list)
19:10:28.53 +25:43:55.9 -- not an asteroid (will add it to exclusion list)
18:50:46.51 +20:52:25.8 -- not an asteroid (will add it to exclusion list)
19:12:46.73 +19:31:41.7 -- not an asteroid (will add it to exclusion list)
19:26:27.15 +21:54:37.6 -- not an asteroid (will add it to exclusion list)
19:10:45.25 +24:37:51.3 -- not an asteroid (will add it to exclusion list)
19:00:04.96 +21:11:47.5 -- not an asteroid (will add it to exclusion list)
19:11:10.27 +19:26:32.1 -- not an asteroid (will add it to exclusion list)
19:13:27.45 +19:56:12.9 -- not an asteroid (will add it to exclusion list)
19:11:28.80 +25:39:16.6 -- not an asteroid (will add it to exclusion list)
19:14:56.57 +24:59:41.7 -- not an asteroid (will add it to exclusion list)
19:17:19.37 +18:22:16.5 -- not an asteroid (will add it to exclusion list)
19:05:23.82 +19:44:23.9 -- not an asteroid (will add it to exclusion list)
19:24:05.81 +26:32:44.3 -- not an asteroid (will add it to exclusion list)
19:12:14.83 +20:15:55.0 -- not an asteroid (will add it to exclusion list)
19:22:55.04 +24:09:57.5 -- not an asteroid (will add it to exclusion list)
19:16:11.78 +25:02:27.7 -- not an asteroid (will add it to exclusion list)
19:09:14.98 +19:23:11.5 -- not an asteroid (will add it to exclusion list)
19:25:28.98 +24:17:10.1 -- not an asteroid (will add it to exclusion list)
19:42:53.52 +25:50:57.5 -- not an asteroid (will add it to exclusion list)
19:43:53.74 +21:01:40.8 -- not an asteroid (will add it to exclusion list)
19:07:08.11 +18:59:17.0 -- not an asteroid (will add it to exclusion list)
18:59:33.41 +25:19:57.2 -- not an asteroid (will add it to exclusion list)
19:11:16.89 +17:51:52.5 -- not an asteroid (will add it to exclusion list)
19:41:49.63 +26:10:38.7 -- not an asteroid (will add it to exclusion list)
19:09:06.61 +24:55:01.5 -- not an asteroid (will add it to exclusion list)
19:17:02.90 +21:30:04.1 -- not an asteroid (will add it to exclusion list)
19:31:55.92 +26:11:20.9 -- not an asteroid (will add it to exclusion list)
19:20:26.46 +25:52:12.4 -- not an asteroid (will add it to exclusion list)
19:10:00.84 +24:22:08.4 -- not an asteroid (will add it to exclusion list)
19:21:45.26 +24:11:49.1 -- not an asteroid (will add it to exclusion list)
19:16:02.54 +24:59:07.1 -- not an asteroid (will add it to exclusion list)
19:14:01.25 +22:32:19.9 -- not an asteroid (will add it to exclusion list)
19:34:11.94 +19:58:28.2 -- not an asteroid (will add it to exclusion list)
19:20:35.75 +26:05:56.7 -- not an asteroid (will add it to exclusion list)
19:20:10.97 +21:17:23.2 -- not an asteroid (will add it to exclusion list)
19:20:55.77 +18:47:27.5 -- not an asteroid (will add it to exclusion list)
19:12:10.30 +24:18:34.4 -- not an asteroid (will add it to exclusion list)
19:13:41.77 +26:37:44.3 -- not an asteroid (will add it to exclusion list)
19:04:31.95 +26:09:09.7 -- not an asteroid (will add it to exclusion list)
19:17:52.50 +19:05:42.0 -- not an asteroid (will add it to exclusion list)
19:23:04.43 +18:35:57.1 -- not an asteroid (will add it to exclusion list)
19:14:41.04 +19:15:01.6 -- not an asteroid (will add it to exclusion list)
19:35:19.57 +17:24:41.7 -- not an asteroid (will add it to exclusion list)
18:57:41.63 +23:24:27.7 -- not an asteroid (will add it to exclusion list)
19:07:08.69 +25:24:15.4 -- not an asteroid (will add it to exclusion list)
19:08:01.85 +24:09:34.7 -- not an asteroid (will add it to exclusion list)
19:10:15.92 +18:48:39.0 -- not an asteroid (will add it to exclusion list)
19:13:46.16 +23:09:28.1 -- not an asteroid (will add it to exclusion list)
19:04:12.03 +25:17:58.8 -- not an asteroid (will add it to exclusion list)
19:04:13.03 +23:58:52.3 -- not an asteroid (will add it to exclusion list)
19:31:02.92 +24:48:43.5 -- not an asteroid (will add it to exclusion list)
18:56:24.44 +22:00:30.1 -- not an asteroid (will add it to exclusion list)
19:24:49.77 +21:56:45.4 -- not an asteroid (will add it to exclusion list)
19:30:31.21 +24:53:03.7 -- not an asteroid (will add it to exclusion list)
19:00:55.84 +24:14:59.4 -- not an asteroid (will add it to exclusion list)
19:02:35.08 +19:11:56.7 -- not an asteroid (will add it to exclusion list)
19:31:11.12 +26:10:51.4 -- not an asteroid (will add it to exclusion list)
19:12:05.80 +26:43:15.3 -- not an asteroid (will add it to exclusion list)
19:12:07.45 +18:44:50.5 -- not an asteroid (will add it to exclusion list)
19:22:00.22 +20:16:29.2 -- not an asteroid (will add it to exclusion list)
19:04:36.17 +24:48:39.8 -- not an asteroid (will add it to exclusion list)
19:30:53.51 +26:39:50.1 -- not an asteroid (will add it to exclusion list)
19:23:14.09 +24:27:38.1 -- not an asteroid (will add it to exclusion list)
19:22:04.22 +20:14:03.6 -- not an asteroid (will add it to exclusion list)
19:23:07.44 +19:28:30.4 -- not an asteroid (will add it to exclusion list)
19:18:23.45 +20:44:33.1 -- not an asteroid (will add it to exclusion list)
19:05:16.09 +22:51:13.2 -- not an asteroid (will add it to exclusion list)
19:24:22.28 +22:48:54.0 -- not an asteroid (will add it to exclusion list)
19:07:35.33 +19:51:27.0 -- not an asteroid (will add it to exclusion list)
19:20:10.34 +20:06:48.5 -- not an asteroid (will add it to exclusion list)
19:14:22.83 +22:22:29.7 -- not an asteroid (will add it to exclusion list)
18:55:46.19 +22:42:45.2 -- not an asteroid (will add it to exclusion list)
19:12:04.80 +18:50:25.1 -- not an asteroid (will add it to exclusion list)
18:54:10.89 +21:29:23.6 -- not an asteroid (will add it to exclusion list)
19:01:55.84 +19:53:52.5 -- not an asteroid (will add it to exclusion list)
19:08:11.28 +22:28:15.7 -- not an asteroid (will add it to exclusion list)
19:15:27.07 +24:45:21.9 -- not an asteroid (will add it to exclusion list)
19:00:27.72 +24:43:46.3 -- not an asteroid (will add it to exclusion list)
19:46:47.03 +18:01:59.9 -- not an asteroid (will add it to exclusion list)
19:03:43.93 +25:59:04.1 -- not an asteroid (will add it to exclusion list)
18:50:51.69 +20:11:21.2 -- not an asteroid (will add it to exclusion list)
19:09:56.06 +22:44:17.5 -- not an asteroid (will add it to exclusion list)
19:06:44.52 +23:13:33.0 -- not an asteroid (will add it to exclusion list)
19:39:20.36 +26:34:31.1 -- not an asteroid (will add it to exclusion list)
19:48:11.32 +26:43:32.3 -- not an asteroid (will add it to exclusion list)
19:20:38.86 +19:09:45.6 -- not an asteroid (will add it to exclusion list)
19:09:45.51 +24:01:34.9 -- not an asteroid (will add it to exclusion list)
19:04:45.78 +26:35:53.3 -- not an asteroid (will add it to exclusion list)
19:09:59.05 +26:11:25.6 -- not an asteroid (will add it to exclusion list)
19:24:07.20 +23:59:24.5 -- not an asteroid (will add it to exclusion list)
19:16:30.20 +25:16:30.4 -- not an asteroid (will add it to exclusion list)
19:08:35.55 +19:29:07.5 -- not an asteroid (will add it to exclusion list)
19:02:36.44 +21:09:36.7 -- not an asteroid (will add it to exclusion list)
19:13:43.42 +18:52:08.2 -- not an asteroid (will add it to exclusion list)
19:05:02.23 +18:38:05.2 -- not an asteroid (will add it to exclusion list)
19:16:20.28 +26:21:24.3 -- not an asteroid (will add it to exclusion list)
19:22:11.80 +17:44:10.2 -- not an asteroid (will add it to exclusion list)
19:05:42.92 +20:31:51.8 -- not an asteroid (will add it to exclusion list)
18:51:42.33 +20:47:54.9 -- not an asteroid (will add it to exclusion list)
19:01:16.48 +18:03:00.1 -- not an asteroid (will add it to exclusion list)
19:05:07.40 +22:24:35.3 -- not an asteroid (will add it to exclusion list)
19:12:40.49 +20:26:28.9 -- not an asteroid (will add it to exclusion list)
19:23:42.39 +22:27:26.1 -- not an asteroid (will add it to exclusion list)
19:16:46.42 +22:16:41.1 -- not an asteroid (will add it to exclusion list)
19:16:56.80 +21:23:28.5 -- not an asteroid (will add it to exclusion list)
18:50:58.78 +20:11:35.6 -- not an asteroid (will add it to exclusion list)
19:22:01.80 +19:17:34.6 -- not an asteroid (will add it to exclusion list)
19:24:47.32 +20:32:41.6 -- not an asteroid (will add it to exclusion list)
19:07:00.45 +20:14:09.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:50:46.51 +20:52:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:46.82 +18:29:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:51.69 +20:11:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:58.78 +20:11:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:42.33 +20:47:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:56.48 +21:48:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:02.65 +23:01:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:10.89 +21:29:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:24.04 +23:33:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:25.62 +22:25:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:46.19 +22:42:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:17.36 +19:28:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:24.44 +22:00:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:57:38.82 +23:40:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:57:41.63 +23:24:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:57:56.52 +21:21:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:45.23 +25:27:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:55.16 +22:29:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:33.41 +25:19:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:52.04 +21:30:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:04.96 +21:11:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:27.72 +24:43:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:55.84 +24:14:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:00.32 +18:41:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:04.19 +25:18:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:16.48 +18:03:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:19.68 +20:28:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:48.83 +21:46:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:55.84 +19:53:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:35.08 +19:11:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:36.44 +21:09:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:38.51 +22:49:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:51.26 +25:24:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:17.58 +20:03:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:43.93 +25:59:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:12.03 +25:17:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:13.03 +23:58:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:31.95 +26:09:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:33.28 +24:40:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:34.08 +25:57:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:36.17 +24:48:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:37.40 +22:16:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:40.56 +26:45:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:45.78 +26:35:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:02.23 +18:38:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:07.40 +22:24:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:16.09 +22:51:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:23.82 +19:44:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:42.92 +20:31:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:18.03 +23:50:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:44.52 +23:13:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:00.45 +20:14:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:08.11 +18:59:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:08.69 +25:24:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:35.33 +19:51:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:01.85 +24:09:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:11.28 +22:28:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:35.55 +19:29:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:06.61 +24:55:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:13.19 +22:04:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:13.44 +23:42:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:14.98 +19:23:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:27.26 +18:49:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:27.93 +24:15:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:43.79 +20:09:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:45.51 +24:01:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:56.06 +22:44:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:59.05 +26:11:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:00.84 +24:22:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:07.59 +20:53:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:15.92 +18:48:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:20.17 +18:59:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:23.03 +24:24:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:28.53 +25:43:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:34.16 +19:11:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:39.39 +19:03:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:45.25 +24:37:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:08.80 +20:07:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:10.27 +19:26:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:15.58 +23:01:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:16.89 +17:51:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:21.37 +25:55:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:28.80 +25:39:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:29.36 +19:39:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:46.21 +24:43:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:01.63 +24:43:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:04.80 +18:50:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:05.80 +26:43:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:07.45 +18:44:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:07.74 +24:36:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:10.30 +24:18:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:14.83 +20:15:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:15.22 +21:20:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:40.49 +20:26:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:41.16 +23:14:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:46.73 +19:31:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:48.22 +24:12:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:49.22 +17:56:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:02.37 +21:28:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:06.67 +20:14:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:15.22 +19:43:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:27.45 +19:56:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:34.95 +26:22:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:41.77 +26:37:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:42.11 +23:43:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:43.42 +18:52:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:46.16 +23:09:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:01.25 +22:32:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:22.83 +22:22:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:41.04 +19:15:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:44.03 +18:56:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:52.38 +23:17:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:56.57 +24:59:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:03.21 +22:56:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:05.14 +19:15:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:27.07 +24:45:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:27.13 +23:28:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:37.49 +24:12:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:54.02 +23:41:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:00.88 +26:44:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:02.54 +24:59:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:11.78 +25:02:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:20.28 +26:21:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:30.20 +25:16:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:46.42 +22:16:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:56.80 +21:23:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:58.11 +17:56:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:02.90 +21:30:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:19.37 +18:22:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:29.24 +25:21:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:29.53 +24:16:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:36.52 +26:01:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:52.50 +19:05:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:59.22 +17:31:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:59.97 +22:31:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:18:05.50 +24:44:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:18:23.45 +20:44:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:18:46.36 +16:59:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:27.87 +24:26:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:51.09 +21:19:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:56.96 +17:07:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:10.34 +20:06:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:10.97 +21:17:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:23.11 +24:24:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:26.46 +25:52:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:35.75 +26:05:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:38.86 +19:09:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:55.77 +18:47:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:02.45 +25:23:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:09.97 +19:48:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:09.98 +26:31:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:38.56 +25:05:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:40.69 +23:13:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:43.99 +24:02:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:45.26 +24:11:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:48.73 +23:35:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:00.22 +20:16:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:01.80 +19:17:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:04.22 +20:14:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:11.80 +17:44:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:55.04 +24:09:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:04.43 +18:35:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:06.05 +22:46:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:07.44 +19:28:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:14.09 +24:27:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:27.89 +25:05:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:42.39 +22:27:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:43.61 +25:03:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:05.81 +26:32:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:05.92 +23:43:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:07.20 +23:59:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:22.28 +22:48:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:43.81 +20:56:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:47.32 +20:32:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:49.77 +21:56:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:28.98 +24:17:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:05.19 +17:26:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:16.91 +18:00:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:25.48 +22:35:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:27.15 +21:54:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:41.80 +24:12:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:54.27 +23:40:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:18.11 +22:21:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:43.61 +26:08:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:28:32.61 +22:12:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:31.21 +24:53:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:53.51 +26:39:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:02.92 +24:48:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:11.12 +26:10:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:30.63 +26:07:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:32.56 +19:49:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:34.02 +19:54:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:50.37 +22:57:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:55.92 +26:11:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:37.28 +23:50:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:51.16 +21:39:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:24.58 +24:18:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:34.37 +26:01:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:11.94 +19:58:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:19.57 +17:24:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:36.39 +21:46:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:38.44 +18:13:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:37.67 +25:17:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:46.07 +25:24:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:10.15 +18:11:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:20.76 +24:43:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:17.76 +18:21:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:20.36 +26:34:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:21.13 +26:18:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:34.48 +23:58:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:36.73 +25:02:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:49.63 +26:10:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:36.43 +25:08:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:53.52 +25:50:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:53.74 +21:01:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:53.21 +24:17:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:06.35 +18:22:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:50.07 +26:44:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:47.03 +18:01:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:11.32 +26:43:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:13.65 +26:35:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:25.63 +23:27:13.8 -- 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)
18:50:46.51 +20:52:25.8 -- a known variable star
18:50:46.82 +18:29:26.7 -- a known variable star
18:50:51.69 +20:11:21.2 -- a known variable star
18:50:58.78 +20:11:35.6 -- a known variable star
18:51:42.33 +20:47:54.9 -- a known variable star
18:51:56.48 +21:48:11.3 -- a known variable star
18:53:02.65 +23:01:35.7 -- a known variable star
18:54:10.89 +21:29:23.6 -- a known variable star
18:54:24.04 +23:33:16.1 -- not a known variable star
18:55:25.62 +22:25:43.9 -- a known variable star
18:55:46.19 +22:42:45.2 -- a known variable star
18:56:17.36 +19:28:47.5 -- a known variable star
18:56:24.44 +22:00:30.1 -- a known variable star
18:57:38.82 +23:40:46.4 -- a known variable star
18:57:41.63 +23:24:27.7 -- a known variable star
18:57:56.52 +21:21:20.1 -- a known variable star
18:58:45.23 +25:27:15.4 -- a known variable star
18:58:55.16 +22:29:54.0 -- a known variable star
18:59:33.41 +25:19:57.2 -- a known variable star
18:59:52.04 +21:30:00.8 -- a known variable star
19:00:04.96 +21:11:47.5 -- a known variable star
19:00:27.72 +24:43:46.3 -- a known variable star
19:00:55.84 +24:14:59.4 -- a known variable star
19:01:00.32 +18:41:45.8 -- a known variable star
19:01:04.19 +25:18:27.2 -- a known variable star
19:01:16.48 +18:03:00.1 -- a known variable star
19:01:19.68 +20:28:27.5 -- a known variable star
19:01:48.83 +21:46:54.5 -- a known variable star
19:01:55.84 +19:53:52.5 -- a known variable star
19:02:35.08 +19:11:56.7 -- a known variable star
19:02:36.44 +21:09:36.7 -- a known variable star
19:02:38.51 +22:49:16.6 -- a known variable star
19:02:51.26 +25:24:55.2 -- a known variable star
19:03:17.58 +20:03:09.5 -- a known variable star
19:03:43.93 +25:59:04.1 -- a known variable star
19:04:12.03 +25:17:58.8 -- a known variable star
19:04:13.03 +23:58:52.3 -- a known variable star
19:04:31.95 +26:09:09.7 -- a known variable star
19:04:33.28 +24:40:51.8 -- a known variable star
19:04:34.08 +25:57:43.4 -- a known variable star
19:04:36.17 +24:48:39.8 -- a known variable star
19:04:37.40 +22:16:09.2 -- a known variable star
19:04:40.56 +26:45:09.9 -- a known variable star
19:04:45.78 +26:35:53.3 -- a known variable star
19:05:02.23 +18:38:05.2 -- a known variable star
19:05:07.40 +22:24:35.3 -- a known variable star
19:05:16.09 +22:51:13.2 -- a known variable star
19:05:23.82 +19:44:23.9 -- a known variable star
19:05:42.92 +20:31:51.8 -- a known variable star
19:06:18.03 +23:50:04.4 -- a known variable star
19:06:44.52 +23:13:33.0 -- a known variable star
19:07:00.45 +20:14:09.9 -- a known variable star
19:07:08.11 +18:59:17.0 -- a known variable star
19:07:08.69 +25:24:15.4 -- a known variable star
19:07:35.33 +19:51:27.0 -- a known variable star
19:08:01.85 +24:09:34.7 -- a known variable star
19:08:11.28 +22:28:15.7 -- a known variable star
19:08:35.55 +19:29:07.5 -- a known variable star
19:09:06.61 +24:55:01.5 -- a known variable star
19:09:13.19 +22:04:03.1 -- a known variable star
19:09:13.44 +23:42:57.0 -- a known variable star
19:09:14.98 +19:23:11.5 -- a known variable star
19:09:27.26 +18:49:47.5 -- a known variable star
19:09:27.93 +24:15:29.9 -- a known variable star
19:09:43.79 +20:09:13.8 -- a known variable star
19:09:45.51 +24:01:34.9 -- a known variable star
19:09:56.06 +22:44:17.5 -- a known variable star
19:09:59.05 +26:11:25.6 -- a known variable star
19:10:00.84 +24:22:08.4 -- a known variable star
19:10:07.59 +20:53:42.5 -- a known variable star
19:10:15.92 +18:48:39.0 -- a known variable star
19:10:20.17 +18:59:47.6 -- not a known variable star
19:10:23.03 +24:24:57.2 -- a known variable star
19:10:28.53 +25:43:55.9 -- a known variable star
19:10:34.16 +19:11:06.6 -- a known variable star
19:10:39.39 +19:03:48.4 -- a known variable star
19:10:45.25 +24:37:51.3 -- a known variable star
19:11:08.80 +20:07:04.0 -- a known variable star
19:11:10.27 +19:26:32.1 -- a known variable star
19:11:15.58 +23:01:23.0 -- a known variable star
19:11:16.89 +17:51:52.5 -- a known variable star
19:11:21.37 +25:55:53.5 -- a known variable star
19:11:28.80 +25:39:16.6 -- a known variable star
19:11:29.36 +19:39:17.9 -- a known variable star
19:11:46.21 +24:43:52.8 -- a known variable star
19:12:01.63 +24:43:11.1 -- a known variable star
19:12:04.80 +18:50:25.1 -- a known variable star
19:12:05.80 +26:43:15.3 -- a known variable star
19:12:07.45 +18:44:50.5 -- a known variable star
19:12:07.74 +24:36:54.6 -- a known variable star
19:12:10.30 +24:18:34.4 -- a known variable star
19:12:14.83 +20:15:55.0 -- not a known variable star
19:12:15.22 +21:20:38.1 -- a known variable star
19:12:40.49 +20:26:28.9 -- a known variable star
19:12:41.16 +23:14:43.6 -- a known variable star
19:12:46.73 +19:31:41.7 -- a known variable star
19:12:48.22 +24:12:51.5 -- a known variable star
19:12:49.22 +17:56:29.7 -- a known variable star
19:13:02.37 +21:28:55.4 -- a known variable star
19:13:06.67 +20:14:10.4 -- a known variable star
19:13:15.22 +19:43:07.2 -- a known variable star
19:13:27.45 +19:56:12.9 -- not a known variable star
19:13:34.95 +26:22:44.8 -- a known variable star
19:13:41.77 +26:37:44.3 -- a known variable star
19:13:42.11 +23:43:58.1 -- a known variable star
19:13:43.42 +18:52:08.2 -- a known variable star
19:13:46.16 +23:09:28.1 -- a known variable star
19:14:01.25 +22:32:19.9 -- a known variable star
19:14:22.83 +22:22:29.7 -- a known variable star
19:14:41.04 +19:15:01.6 -- a known variable star
19:14:44.03 +18:56:50.2 -- a known variable star
19:14:52.38 +23:17:46.6 -- a known variable star
19:14:56.57 +24:59:41.7 -- a known variable star
19:15:03.21 +22:56:16.0 -- a known variable star
19:15:05.14 +19:15:09.2 -- a known variable star
19:15:27.07 +24:45:21.9 -- a known variable star
19:15:27.13 +23:28:48.0 -- a known variable star
19:15:37.49 +24:12:07.9 -- a known variable star
19:15:54.02 +23:41:30.6 -- not a known variable star
19:16:00.88 +26:44:19.9 -- a known variable star
19:16:02.54 +24:59:07.1 -- a known variable star
19:16:11.78 +25:02:27.7 -- a known variable star
19:16:20.28 +26:21:24.3 -- a known variable star
19:16:30.20 +25:16:30.4 -- a known variable star
19:16:46.42 +22:16:41.1 -- a known variable star
19:16:56.80 +21:23:28.5 -- a known variable star
19:16:58.11 +17:56:55.6 -- a known variable star
19:17:02.90 +21:30:04.1 -- a known variable star
19:17:19.37 +18:22:16.5 -- a known variable star
19:17:29.24 +25:21:17.2 -- a known variable star
19:17:29.53 +24:16:05.4 -- a known variable star
19:17:36.52 +26:01:42.1 -- a known variable star
19:17:52.50 +19:05:42.0 -- a known variable star
19:17:59.22 +17:31:47.2 -- a known variable star
19:17:59.97 +22:31:43.0 -- a known variable star
19:18:05.50 +24:44:03.7 -- a known variable star
19:18:23.45 +20:44:33.1 -- a known variable star
19:18:46.36 +16:59:32.5 -- a known variable star
19:19:27.87 +24:26:21.3 -- a known variable star
19:19:51.09 +21:19:39.1 -- not a known variable star
19:19:56.96 +17:07:46.7 -- not a known variable star
19:20:10.34 +20:06:48.5 -- a known variable star
19:20:10.97 +21:17:23.2 -- a known variable star
19:20:23.11 +24:24:41.3 -- a known variable star
19:20:26.46 +25:52:12.4 -- a known variable star
19:20:35.75 +26:05:56.7 -- a known variable star
19:20:38.86 +19:09:45.6 -- a known variable star
19:20:55.77 +18:47:27.5 -- a known variable star
19:21:02.45 +25:23:42.5 -- a known variable star
19:21:09.97 +19:48:39.8 -- a known variable star
19:21:09.98 +26:31:01.9 -- a known variable star
19:21:38.56 +25:05:04.8 -- a known variable star
19:21:40.69 +23:13:37.9 -- a known variable star
19:21:43.99 +24:02:05.0 -- a known variable star
19:21:45.26 +24:11:49.1 -- a known variable star
19:21:48.73 +23:35:18.9 -- a known variable star
19:22:00.22 +20:16:29.2 -- a known variable star
19:22:01.80 +19:17:34.6 -- a known variable star
19:22:04.22 +20:14:03.6 -- a known variable star
19:22:11.80 +17:44:10.2 -- a known variable star
19:22:55.04 +24:09:57.5 -- a known variable star
19:23:04.43 +18:35:57.1 -- a known variable star
19:23:06.05 +22:46:36.3 -- a known variable star
19:23:07.44 +19:28:30.4 -- a known variable star
19:23:14.09 +24:27:38.1 -- a known variable star
19:23:27.89 +25:05:34.3 -- a known variable star
19:23:42.39 +22:27:26.1 -- a known variable star
19:23:43.61 +25:03:39.4 -- a known variable star
19:24:05.81 +26:32:44.3 -- a known variable star
19:24:05.92 +23:43:30.8 -- a known variable star
19:24:07.20 +23:59:24.5 -- a known variable star
19:24:22.28 +22:48:54.0 -- a known variable star
19:24:43.81 +20:56:00.4 -- a known variable star
19:24:47.32 +20:32:41.6 -- a known variable star
19:24:49.77 +21:56:45.4 -- a known variable star
19:25:28.98 +24:17:10.1 -- a known variable star
19:26:05.19 +17:26:57.3 -- a known variable star
19:26:16.91 +18:00:18.5 -- a known variable star
19:26:25.48 +22:35:58.4 -- a known variable star
19:26:27.15 +21:54:37.6 -- a known variable star
19:26:41.80 +24:12:26.7 -- a known variable star
19:26:54.27 +23:40:26.7 -- a known variable star
19:27:18.11 +22:21:35.6 -- a known variable star
19:27:43.61 +26:08:30.5 -- a known variable star
19:28:32.61 +22:12:07.1 -- a known variable star
19:30:31.21 +24:53:03.7 -- a known variable star
19:30:53.51 +26:39:50.1 -- a known variable star
19:31:02.92 +24:48:43.5 -- a known variable star
19:31:11.12 +26:10:51.4 -- a known variable star
19:31:30.63 +26:07:04.2 -- a known variable star
19:31:32.56 +19:49:59.7 -- a known variable star
19:31:34.02 +19:54:00.4 -- a known variable star
19:31:50.37 +22:57:36.8 -- a known variable star
19:31:55.92 +26:11:20.9 -- a known variable star
19:32:37.28 +23:50:58.9 -- a known variable star
19:32:51.16 +21:39:03.9 -- a known variable star
19:33:24.58 +24:18:23.9 -- a known variable star
19:33:34.37 +26:01:17.2 -- a known variable star
19:34:11.94 +19:58:28.2 -- a known variable star
19:35:19.57 +17:24:41.7 -- a known variable star
19:35:36.39 +21:46:10.2 -- not a known variable star
19:35:38.44 +18:13:38.0 -- a known variable star
19:36:37.67 +25:17:22.4 -- a known variable star
19:36:46.07 +25:24:56.3 -- a known variable star
19:37:10.15 +18:11:20.3 -- a known variable star
19:38:20.76 +24:43:00.1 -- a known variable star
19:39:17.76 +18:21:34.8 -- a known variable star
19:39:20.36 +26:34:31.1 -- a known variable star
19:39:21.13 +26:18:43.7 -- a known variable star
19:40:34.48 +23:58:08.3 -- a known variable star
19:40:36.73 +25:02:46.0 -- a known variable star
19:41:49.63 +26:10:38.7 -- a known variable star
19:42:36.43 +25:08:47.5 -- a known variable star
19:42:53.52 +25:50:57.5 -- a known variable star
19:43:53.74 +21:01:40.8 -- a known variable star
19:44:53.21 +24:17:36.4 -- a known variable star
19:45:06.35 +18:22:43.0 -- a known variable star
19:45:50.07 +26:44:26.9 -- a known variable star
19:46:47.03 +18:01:59.9 -- a known variable star
19:48:11.32 +26:43:32.3 -- a known variable star
19:52:13.65 +26:35:19.1 -- a known variable star
19:55:25.63 +23:27:13.8 -- a known variable star
Found 8 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
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222 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 222 (excluding asteroids and hot pixels, 8 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)2461348.68002916 -observatory V36
14:38:58.51 -16:02:11.7 Mercury (6.3mag)
13:24:24.87 -13:16:17.3 Venus (-4.4mag)
09:31:09.16 +16:26:50.3 Mars (0.8mag)
09:47:27.25 +14:04:26.9 Jupiter (-2.0mag)
00:36:14.39 +00:59:35.3 Saturn (0.5mag)
04:08:54.29 +20:49:48.0 Uranus (5.6mag)
00:08:16.47 -00:38:38.7 Neptune (7.7mag)
20:24:30.15 -23:41:24.9 Pluto (14.5mag)
10:48:12.96 +05:48:10.0 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 361 Nov 3 22:25 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461348.68002916:
09:47:32.64 +14:03:56.2 Io (6.0mag)
09:47:19.17 +14:05:12.5 Europa (6.1mag)
09:47:30.04 +14:04:11.8 Ganymede (5.5mag)
09:47:58.18 +14:01:31.2 Callisto (6.8mag)
09:48:57.65 +14:13:25.2 Himalia (15.5mag)
09:47:28.28 +14:04:22.3 Thebe (16.3mag)
09:47:16.02 +14:29:29.8 Elara (17.4mag)
09:48:08.86 +13:32:25.0 Pasiphae (17.7mag)
09:44:25.77 +14:36:29.0 Carme (18.7mag)
00:36:25.45 +00:59:11.3 Titan (8.3mag)
00:36:09.29 +00:59:39.4 Rhea (9.6mag)
00:36:45.92 +01:00:23.7 Iapetus (11.0mag)
00:36:06.04 +00:59:10.2 Hyperion (14.2mag)
00:34:27.64 +00:47:27.5 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Nov 3 22:25 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461348.68002916:
04:38:31.58 +17:07:34.9 JWST
17:03:37.94 +40:30:12.1 Chandra
11:11:17.83 -59:37:47.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Nov 3 22:25 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461348.68002916 -observatory V36
03:33:04.81 +19:55:42.0 17.1mag P/1996 R2 (Lagerkvist)
07:46:52.30 +38:26:24.0 17.8mag P/2004 V5 (LINEAR-Hill)
07:46:57.68 +38:26:11.0 17.8mag P/2004 V5-A (LINEAR-Hill)
07:46:16.07 +38:26:31.4 17.8mag P/2004 V5-B (LINEAR-Hill)
05:01:42.64 +38:58:33.3 17.7mag P/2009 Y2 (Kowalski)
18:48:56.56 -32:51:14.3 15.0mag P/2010 H2 (Vales)
07:45:20.60 -73:57:16.8 17.2mag C/2014 UN271 (Bernardinelli-Bernstein)
06:11:16.61 +35:19:46.7 17.7mag C/2017 K2 (PANSTARRS)
07:35:46.49 +25:20:21.9 16.9mag C/2022 N2 (PANSTARRS)
09:08:37.90 +38:38:28.2 16.4mag C/2024 E1 (Wierzchos)
18:37:31.33 +40:51:55.9 17.5mag C/2024 J3 (ATLAS)
05:42:48.19 -13:32:19.1 16.3mag C/2024 T5 (ATLAS)
14:16:07.08 -04:38:49.8 16.3mag C/2025 Y1 (ATLAS)
20:17:38.61 +52:34:57.4 15.2mag C/2026 A2 (Bok)
13:08:18.47 +17:05:38.6 17.7mag A/2026 E1
15:58:43.16 -65:53:29.4 14.6mag P/2026 R2 (Leonard)
19:34:49.33 -05:22:47.7 17.1mag P/2026 T1 (ATLAS)
23:27:07.96 +13:51:30.8 16.8mag 2P/Encke
23:27:03.94 -25:33:36.7 15.4mag 10P/Tempel
02:40:51.10 +30:09:39.2 16.3mag 11P/Tempel-Swift-LINEAR
12:26:38.10 -10:05:52.2 16.3mag 29P/Schwassmann-Wachmann
00:10:25.12 -09:00:32.4 15.9mag 65P/Gunn
08:00:47.25 +13:30:36.1 14.0mag 78P/Gehrels
09:02:18.08 +46:06:50.5 17.1mag 112P/Urata-Niijima
09:52:34.41 +05:18:11.3 17.8mag 114P/Wiseman-Skiff
12:28:21.91 +07:52:33.5 14.8mag 123P/West-Hartley
19:47:12.45 +14:36:45.5 10.2mag 161P/Hartley-IRAS
11:13:45.24 -03:14:33.0 16.3mag 169P/NEAT
09:41:53.49 +23:27:46.2 18.0mag 186P/Garradd
03:09:58.28 +02:08:04.0 15.3mag 220P/McNaught
06:22:41.35 +49:53:57.0 15.6mag 260P/McNaught
07:57:15.70 +25:03:42.4 17.5mag 266P/Christensen
-rw-r--r-- 1 apache apache 1.6K Nov 3 22:25 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
02:29:41.13 -71:57:55.60 ASASSN-26fr 2026-11-1.22 13.7
21:27:22.43 -18:15:42.10 SN 2026agsu 2026-10-29.85 -1.08
17:54:18.84 -27:36:35.70 TCP J17541876-2736362 2026-10-24.76 9.92
10:38:47.97 +53:30:34.00 SN2026sqf 2026-10-24.6 13.27
21:49:53.30 +14:07:44.90 ASASSN-26fq 2026-10-23.23 14.82
01:00:14.36 +34:04:05.90 ASASSN-26fp 2026-10-23.34 12.9
01:06:23.14 -63:46:37.10 ASASSN-26fo 2026-10-19.79 -4.88
00:25:28.03 +20:14:39.10 SN2026afqd 2026-10-19.36 -0.77
22:14:03.37 -45:07:18.60 ASASSN-26fm 2026-10-13.75 14.42
01:57:48.19 -33:14:42.30 SN 2026aedl 2026-10-12.33 15.3
18:05:22.06 +17:52:41.00 ASASSN-26fn 2026-10-11.74 15.23
21:50:55.86 -02:51:49.30 SN2026acyb 2026-10-9.85 16.83
03:40:34.04 +02:31:56.70 SN2026acvp 2026-10-9.95 17.75
04:33:25.91 -13:41:04.20 SN2026adhl 2026-10-9.94 17.52
09:20:05.05 +27:03:12.40 SN2026aeif 2026-10-9.47 15.93
02:58:07.77 -65:18:52.90 ASASSN-26fl 2026-10-7.9 -0.85
02:49:03.98 -49:55:57.00 SN 2026adfy 2026-10-4.88 16.61
22:03:46.31 -11:07:57.70 AT2026adgn 2026-10-4.28 -2.56
15:03:12.98 +49:51:05.40 ASASSN-26fj 2026-10-2.06 15.91
08:07:27.96 -65:51:03.90 ASASSN-26fi 2026-10-1.36 15.82
21:02:34.66 +23:57:26.20 ASASSN-26fh 2026-10-1.27 15.94
20:00:16.62 +03:26:29.90 AT2026adfv 2026-10-1.3 16.42
00:08:42.74 -32:33:16.50 SN2026abhc 2026-09-29.15 15.57
21:02:30.26 -19:27:41.80 SN2026acxa 2026-09-29.13 14.65
04:39:17.45 -28:06:12.40 ASASSN-26fg 2026-09-23.25 15.73
05:25:07.80 +04:38:32.40 SN2026aajs 2026-09-21.32 17.04
19:56:12.67 +08:25:27.70 AT2026acgs 2026-09-18.14 15.84
00:02:34.06 +52:55:18.90 ASASSN-26ff 2026-09-16.38 15.41
23:44:33.18 +17:46:12.20 SN2026yjv 2026-09-15.38 18.32
16:21:12.24 +57:37:51.30 SN 2026aafh 2026-09-14.11 15.02
23:36:00.27 -19:28:18.00 SN 2026aaks 2026-09-14.44 16.89
16:35:24.86 -05:32:38.20 SN2026aasi 2026-09-12.99 16.58
16:46:08.71 +37:25:21.80 SN2026aafk 2026-09-13.25 17.4
23:48:37.86 +50:25:24.60 SN2026aafs 2026-09-13.47 17
21:20:27.02 +02:10:42.50 SN2026aagh -------
08:02:26.85 -24:37:44.10 ASASSN-26fe 2026-09-13.34 13.67
02:29:34.91 +23:06:56.30 SN2026aars 2026-09-12.27 16.93
02:47:25.52 -32:58:34.50 SN 2026znh 2026-09-9.92 16.26
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc 2026-09-8.79 12.14
03:52:53.26 -14:19:28.70 SN 2026zfw 2026-09-8 17.78
01:53:26.46 +10:07:25.10 SN2026aacj 2026-09-7.17 16.27
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.64 +34:24:35.00 SN2026aaiv 2026-09-7.25 13.48
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa 2026-08-31.18 14.63
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
-rw-r--r-- 1 apache apache 5.7K Nov 3 22:25 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
00:42:40.94 +41:15:37.1 PNV J00424094+4115371 2026-09-17.8925 18.3mag
08:49:20.13 -09:19:15.8 TCP J08492013-0919158 2026-09-18.4698 13.3mag
00:42:13.93 +41:16:35.6 PNV J00421393+4116356 2026-09-22.6597 19.66Cmag
18:14:01.58 +15:13:55.5 TCP J18140158+1513555 2026-09-24.4645 14.1mag
00:42:36.61 +41:13:50.5 TCP J00423661+4113505 2026-09-29.7462 17.4mag
22:03:46.29 -11:07:57.8 TCP J22034629-1107578 2026-09-29.7438 14.51Cmag
22:05:02.06 +20:49:01.2 TCP J22050206+2049012 2026-10-03.5715 17.13Cmag
00:38:15.01 +41:14:47.2 TCP J00381501+4114472 2026-10-08.5978 17.72Cmag
01:06:05.83 +09:51:20.4 TCP J01060583+0951204 2026-10-10.8543 14.54Cmag
17:54:18.76 -27:36:36.2 TCP J17541876-2736362 2026-10-12.3993 10.8mag
09:56:00.79 +69:06:15.2 PNV J09560079+6906152 2026-10-14.9274 19.38Cmag
00:43:30.83 +41:26:55.3 PNV J00433083+4126553 2026-10-17.5651 18.61Cmag
04:57:32.08 +30:15:41.6 TCP J04573208+3015416 2026-10-17.7818 18.21Cmag
05:21:07.64 +23:38:21.3 TCP J05210764+2338213 2026-10-18.4020 10.3mag
05:34:11.01 +28:45:30.5 TCP J05341101+2845305 2026-10-18.3604 16.6mag
-rw-r--r-- 1 apache apache 191K Nov 3 22:25 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:49:07.467 +20:28:27.00 AT 2026afvq 2026-10-18.54 19.0025
05:21:07.640 +23:38:21.30 AT 2026afvp 2026-10-18.40 10.3
09:31:51.300 -05:51:50.06 AT 2026afvo 2026-10-18.53 19.3989
11:47:33.570 +15:53:59.36 AT 2026afvn 2026-10-18.54 17.9673
04:08:22.865 -01:57:41.49 AT 2026afvm 2026-10-03.57 20.74
02:57:23.229 +23:15:05.14 AT 2026afvl 2026-10-14.38 21.6
03:39:38.127 +00:06:23.78 AT 2026afvk 2026-10-03.54 20.86
06:28:56.066 -21:10:56.44 AT 2026afvj 2026-10-17.61 20.66
22:36:58.814 +12:17:43.08 AT 2026afvi 2026-10-18.22 20.88
22:19:44.739 +14:32:54.10 AT 2026afvh 2026-10-18.22 21.11
03:33:51.668 +02:12:48.26 AT 2026afvg 2026-10-18.34 20.3423
01:50:59.284 -14:35:47.52 AT 2026afvf 2026-10-15.29 19.8509
03:33:40.648 +03:15:42.84 AT 2026afve 2026-10-18.41 20.2098
05:47:54.576 +66:31:16.59 AT 2026afvd 2026-10-15.40 19.7645
01:21:24.040 +10:11:02.74 AT 2026afvc 2026-10-13.74 21.71
00:04:52.660 +28:32:15.80 AT 2026afvb 2026-10-13.53 19.96
23:32:22.880 +13:42:51.02 AT 2026afva 2026-10-17.77 20.92
07:39:44.850 +58:14:11.33 AT 2026afuz 2026-10-08.88 21.51
23:05:43.620 +33:22:00.16 AT 2026afuy 2026-10-08.85 21.74
23:59:42.800 +15:17:57.90 AT 2026afux 2026-10-05.79 21.82
-rw-r--r-- 1 apache apache 89K Nov 3 22:25 tns_transients_list.txt
