This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461274.8960,6.46,0.05,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
VARIABLE_NAME 20260822.3960 6.46CV 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 08 22.3960 2461274.8960 9.65 06:13:44.33 +22:34:55.6
188.66153 2.32323 galactic Gem Second-epoch detections are separated by 0.9" and 9.5 pix
The object was found in VSX17" ZTF J061344.23+223438.6
Type: EA
# Max. Min./Amp. JD0 Period
17.727 r Y 0.556 r 2458457.77270 0.477039800000
NOTE: the measured brightness disagrees with the variable-star record above, but is consistent with the asteroid identification below - so this is likely the asteroid rather than an outburst of the variable.
The object was found in astcheck.1 Ceres 0 0 0 8.9 -0 -0
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:13:44.33 +22:34:55.6: 14.55 +/- 0.11 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:13:44.33 +22:34:55.6: 14.36 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.44 +/- 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 J061344.23+223438.6,2461274.8960,9.65,0.05,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 J061344.23+223438.6 20260822.3960 9.65CV 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 08 22.3960 2461274.8960 9.51 06:37:19.81 +18:12:48.3
195.10910 5.19318 galactic Gem Second-epoch detections are separated by 1.0" and 9.8 pix
The object was found in VSX 0" EQ Gem
Type: LB
# Max. Min./Amp. JD0 Period
10.560 V Y 0.220 V 2452726.50000 39.066167000000 M0
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:37:19.81 +18:12:48.3: 10.30 +/- 0.00 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:37:19.81 +18:12:48.3: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.42 +/- 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
EQ Gem,2461274.8960,9.51,0.05,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
EQ Gem 20260822.3960 9.51CV 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 08 22.3960 2461274.8960 9.61 06:29:39.75 +17:18:08.9
195.08575 3.15310 galactic Gem Second-epoch detections are separated by 1.0" and 9.8 pix
The object was found in VSX 1" NSV 2982
Type: LB
# Max. Min./Amp. JD0 Period
11.310 V Y 0.120 V 2452683.90000 37.429778000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:39.75 +17:18:08.9: 10.61 +/- 0.00 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:39.75 +17:18:08.9: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.56 +/- 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
NSV 2982,2461274.8960,9.61,0.05,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
NSV 2982 20260822.3960 9.61CV 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 08 22.3960 2461274.8960 11.34 05:58:53.45 +24:23:03.7
185.42664 0.23066 galactic Tau Second-epoch detections are separated by 0.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.22 Kalliope -0 -0 1 12.2 -0 -0
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:58:53.45 +24:23:03.7: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:58:53.45 +24:23:03.7: 15.73 +/- 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!
TCP 2026 08 22.3960* 05 58 53.45 +24 23 03.7 11.3 U Tau 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
VARIABLE_NAME,2461274.8960,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260822.3960 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 10.38 06:37:01.57 +18:31:41.3
194.79446 5.27112 galactic Gem Second-epoch detections are separated by 0.6" and 9.9 pix
The object was found in VSX 0" ASAS J063702+1831.7
Type: MISC
# Max. Min./Amp. JD0 Period
11.470 V Y 0.290 V 2452813.80000 81.365512000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:37:01.57 +18:31:41.3: 11.26 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:37:01.57 +18:31:41.3: 11.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 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 J063702+1831.7,2461274.8960,10.38,0.05,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
ASAS J063702+1831.7 20260822.3960 10.38CV 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 08 22.3960 2461274.8960 10.53 06:35:11.51 +21:03:38.5
192.32782 6.02923 galactic Gem Second-epoch detections are separated by 0.8" and 9.9 pix
The object was found in VSX 1" ASAS J063511+2103.6
Type: MISC
# Max. Min./Amp. JD0 Period
11.890 V Y 0.630 V 2452840.30000 89.200000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:35:11.51 +21:03:38.5: 11.63 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:35:11.51 +21:03:38.5: 11.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J063511+2103.6,2461274.8960,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J063511+2103.6 20260822.3960 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.20 06:27:51.95 +18:29:51.4
193.82626 3.32572 galactic Gem Second-epoch detections are separated by 3.8" and 10.3 pix
The object was found in VSX 3" ASASSN-V J062752.14+182952.3
Type: SR
# Max. Min./Amp. JD0 Period
12.870 V 13.400 V 2457469.80000 91.700000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:27:51.95 +18:29:51.4: 12.25 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:27:51.95 +18:29:51.4: 12.05 +/- 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
ASASSN-V J062752.14+182952.3,2461274.8960,11.20,0.05,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 J062752.14+182952.3 20260822.3960 11.20CV 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 08 22.3960 2461274.8960 11.52 06:32:34.66 +19:06:36.0
193.79430 4.59749 galactic Gem Second-epoch detections are separated by 1.2" and 9.9 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 | DocumentRef: VOTx2592397 | 06:32:34.72 +19:06:36.2 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE J-Ks=1.268+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:32:34.66 +19:06:36.0: 12.42 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:32:34.66 +19:06:36.0: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2592397,2461274.8960,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2592397 20260822.3960 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.47 06:28:54.02 +17:18:25.7
194.99751 2.99388 galactic Gem Second-epoch detections are separated by 1.3" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.2334+17.2995 | 06:28:53.96 +17:18:24.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.788+/-0.027 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:54.02 +17:18:25.7: 12.46 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:54.02 +17:18:25.7: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.2334+17.2995,2461274.8960,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.2334+17.2995 20260822.3960 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.76 05:56:31.67 +23:57:33.3
185.52481 -0.44871 galactic Tau Second-epoch detections are separated by 2.5" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3427849888980635776 | 05:56:31.71 +23:57:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.809+/-0.027 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:56:31.67 +23:57:33.3: 12.67 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:56:31.67 +23:57:33.3: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 08 22.3960* 05 56 31.67 +23 57 33.3 11.8 U Tau 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
Gaia DR3 3427849888980635776,2461274.8960,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3427849888980635776 20260822.3960 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.70 06:32:05.70 +19:05:40.0
193.75596 4.48895 galactic Gem Second-epoch detections are separated by 1.4" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3371471468194871424 | 06:32:05.69 +19:05:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.643+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:32:05.70 +19:05:40.0: 12.69 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:32:05.70 +19:05:40.0: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3371471468194871424,2461274.8960,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3371471468194871424 20260822.3960 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.70 06:01:01.75 +26:26:14.7
183.88476 1.66995 galactic Gem Second-epoch detections are separated by 2.1" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.2573+26.4375 | 06:01:01.75 +26:26:15.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.273+/-0.038 (Very red! L if it's a dwarf)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:01:01.75 +26:26:14.7: 12.72 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:01:01.75 +26:26:14.7: 12.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.2573+26.4375,2461274.8960,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.2573+26.4375 20260822.3960 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.68 06:31:54.44 +20:02:00.3
192.89746 4.87818 galactic Gem Second-epoch detections are separated by 2.1" and 9.8 pix
The object was found in VSX 1" ASASSN-V J063154.49+200200.4
Type: SRS
# Max. Min./Amp. JD0 Period
13.900 g Y 0.190 g 2459148.93700 28.068000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:31:54.44 +20:02:00.3: 12.78 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:31:54.44 +20:02:00.3: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 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 J063154.49+200200.4,2461274.8960,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063154.49+200200.4 20260822.3960 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.96 06:31:50.45 +20:03:28.2
192.86850 4.87542 galactic Gem Second-epoch detections are separated by 2.0" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:31:50.45 +20:03:28.2 (user input) | T | P | (position from user input) J-Ks=0.690+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:31:50.45 +20:03:28.2: 13.07 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:31:50.45 +20:03:28.2: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8960,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3960 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 08 22.3960 2461274.8960 11.76 06:20:34.93 +18:19:55.9
193.16614 1.72032 galactic Gem Second-epoch detections are separated by 0.8" and 9.6 pix
The object was found in VSX 1" ASASSN-V J062034.87+181955.8
Type: SR
# Max. Min./Amp. JD0 Period
13.320 V 13.740 V 2457669.10000 68.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:20:34.93 +18:19:55.9: 12.93 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:20:34.93 +18:19:55.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062034.87+181955.8,2461274.8960,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062034.87+181955.8 20260822.3960 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.39 06:34:56.99 +22:45:02.8
190.78330 6.73884 galactic Gem Second-epoch detections are separated by 2.9" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.27 Euterpe 0 1 1 11.5 0 0
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:34:56.99 +22:45:02.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:34:56.99 +22:45:02.8: 15.82 +/- 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
VARIABLE_NAME,2461274.8960,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260822.3960 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.74 06:29:00.04 +18:13:51.3
194.18777 3.44145 galactic Gem Second-epoch detections are separated by 2.9" and 9.8 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 | DocumentRef: VOTx2717804 | 06:29:00.04 +18:13:51.3 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.783+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:00.04 +18:13:51.3: 12.89 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:00.04 +18:13:51.3: 12.94 +/- 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
DocumentRef: VOTx2717804,2461274.8960,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2717804 20260822.3960 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.84 06:29:25.55 +18:59:03.0
193.56429 3.87779 galactic Gem Second-epoch detections are separated by 2.4" and 10.1 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 | DocumentRef: VOTx2663137 | 06:29:25.59 +18:59:03.6 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=1.238+/-0.026 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:25.55 +18:59:03.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:25.55 +18:59:03.0: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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
DocumentRef: VOTx2663137,2461274.8960,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2663137 20260822.3960 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.78 06:31:15.57 +17:46:35.4
194.83960 3.70921 galactic Gem Second-epoch detections are separated by 2.8" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3371229957891331968 | 06:31:15.63 +17:46:35.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.178+/-0.025 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:31:15.57 +17:46:35.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:31:15.57 +17:46:35.4: 12.87 +/- 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
Gaia DR3 3371229957891331968,2461274.8960,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3371229957891331968 20260822.3960 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.67 06:28:12.19 +17:12:32.3
195.00761 2.80090 galactic Gem Second-epoch detections are separated by 2.2" and 9.7 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 | 06:28:12.19 +17:12:32.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:12.19 +17:12:32.3: 12.84 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:12.19 +17:12:32.3: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8960,11.67,0.05,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
target 20260822.3960 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 08 22.3960 2461274.8960 11.84 06:32:34.56 +20:06:35.4
192.90097 5.05277 galactic Gem Second-epoch detections are separated by 0.1" and 9.8 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 | 06:32:34.56 +20:06:35.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.715+/-0.027 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:32:34.56 +20:06:35.4: 12.81 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:32:34.56 +20:06:35.4: 12.82 +/- 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
target,2461274.8960,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3960 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.65 06:29:14.49 +17:37:51.4
194.74747 3.21553 galactic Gem Second-epoch detections are separated by 0.7" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.3104+17.6310 | 06:29:14.52 +17:37:51.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.151+/-0.027 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:14.49 +17:37:51.4: 12.79 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:14.49 +17:37:51.4: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.3104+17.6310,2461274.8960,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.3104+17.6310 20260822.3960 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.74 06:28:24.96 +18:12:14.3
194.14753 3.30584 galactic Gem Second-epoch detections are separated by 2.4" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.1038+18.2040 | 06:28:24.92 +18:12:14.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=1.306+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:24.96 +18:12:14.3: 12.75 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:24.96 +18:12:14.3: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.1038+18.2040,2461274.8960,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.1038+18.2040 20260822.3960 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.68 06:29:05.33 +18:07:42.3
194.28856 3.41276 galactic Gem Second-epoch detections are separated by 3.0" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3371314444190561536 | 06:29:05.35 +18:07:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.230+/-0.028 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:05.33 +18:07:42.3: 12.77 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:05.33 +18:07:42.3: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3371314444190561536,2461274.8960,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3371314444190561536 20260822.3960 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.64 06:35:46.76 +17:44:27.1
195.36414 4.65028 galactic Gem Second-epoch detections are separated by 2.3" and 9.4 pix
The object was found in VSX 0" ASASSN-V J063546.74+174427.2
Type: SR
# Max. Min./Amp. JD0 Period
14.050 g Y 0.190 g 2459316.53700 44.720000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:35:46.76 +17:44:27.1: 12.75 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:35:46.76 +17:44:27.1: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063546.74+174427.2,2461274.8960,11.64,0.05,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 J063546.74+174427.2 20260822.3960 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 08 22.3960 2461274.8960 11.71 06:33:56.06 +19:46:04.3
193.35247 5.18169 galactic Gem Second-epoch detections are separated by 2.6" and 9.7 pix
The object was found in VSX20" KELT KC04C002559
Type: EA
# Max. Min./Amp. JD0 Period
10.950 V Y 0.007 i 2455958.63600 2.643460000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:33:56.06 +19:46:04.3: 12.75 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:33:56.06 +19:46:04.3: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KELT KC04C002559,2461274.8960,11.71,0.05,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
KELT KC04C002559 20260822.3960 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 08 22.3960 2461274.8960 11.69 06:38:01.65 +18:48:00.2
194.65823 5.60548 galactic Gem Second-epoch detections are separated by 1.3" and 9.6 pix
The object was found in VSX 1" ASASSN-V J063801.62+184759.4
Type: SR
# Max. Min./Amp. JD0 Period
12.880 V 12.990 V 2457421.92900 41.690000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:38:01.65 +18:48:00.2: 12.73 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:38:01.65 +18:48:00.2: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 J063801.62+184759.4,2461274.8960,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063801.62+184759.4 20260822.3960 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.73 06:29:34.12 +17:51:36.0
194.57986 3.39027 galactic Gem Second-epoch detections are separated by 4.6" and 10.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:29:34.12 +17:51:36.0 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.207+/-0.031 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:34.12 +17:51:36.0: 12.73 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:34.12 +17:51:36.0: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8960,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3960 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.66 06:29:24.20 +18:15:38.7
194.20539 3.54004 galactic Gem Second-epoch detections are separated by 1.5" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3371323691253552128 | 06:29:24.10 +18:15:39.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.755+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:24.20 +18:15:38.7: 12.72 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:24.20 +18:15:38.7: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 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
Large-amplitude variable Gaia DR2 3371323691253552128,2461274.8960,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3371323691253552128 20260822.3960 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.69 06:28:41.22 +17:07:34.2
195.13464 2.86506 galactic Gem Second-epoch detections are separated by 4.1" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx2980775 | 06:28:41.25 +17:07:34.9 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.886+/-0.044 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:41.22 +17:07:34.2: 12.69 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:41.22 +17:07:34.2: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 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
DocumentRef: VOTx2980775,2461274.8960,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2980775 20260822.3960 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.72 05:56:05.97 +25:30:55.0
184.13090 0.24967 galactic Tau Second-epoch detections are separated by 0.3" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3428290380825674752 | 05:56:05.92 +25:30:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.945+/-0.027 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:56:05.97 +25:30:55.0: 12.72 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:56:05.97 +25:30:55.0: 12.75 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 05 56 05.97 +25 30 55.0 11.7 U Tau 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
Gaia DR3 3428290380825674752,2461274.8960,11.72,0.05,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
Gaia DR3 3428290380825674752 20260822.3960 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 08 22.3960 2461274.8960 11.18 06:27:43.04 +18:57:36.7
193.39902 3.50830 galactic Gem Second-epoch detections are separated by 0.9" and 9.6 pix
The object was found in VSX 1" NSVS 9774104
Type: L
# Max. Min./Amp. JD0 Period
10.300 R1 10.600 R1 M7
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:27:43.04 +18:57:36.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:27:43.04 +18:57:36.7: 12.20 +/- 0.01 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
NSVS 9774104,2461274.8960,11.18,0.05,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
NSVS 9774104 20260822.3960 11.18CV 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 08 22.3960 2461274.8960 11.81 06:00:27.35 +26:26:03.3
183.82390 1.55689 galactic Tau Second-epoch detections are separated by 2.4" and 9.6 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 | DocumentRef: VOTx3408565 | 06:00:27.36 +26:26:03.8 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.915+/-0.028 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:00:27.35 +26:26:03.3: 12.71 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:00:27.35 +26:26:03.3: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 06 00 27.35 +26 26 03.3 11.8 U Tau 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
DocumentRef: VOTx3408565,2461274.8960,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3408565 20260822.3960 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.79 06:34:19.52 +19:51:36.5
193.31178 5.30550 galactic Gem Second-epoch detections are separated by 1.5" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J098.5887+19.8487 | 06:34:19.54 +19:51:35.4 (Gaia DR3) | CBH (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.184+/-0.031 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:34:19.52 +19:51:36.5: 12.70 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:34:19.52 +19:51:36.5: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.5887+19.8487,2461274.8960,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.5887+19.8487 20260822.3960 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 08 22.3960 2461274.8960 11.73 06:27:14.20 +17:29:01.6
194.65683 2.72379 galactic Gem Second-epoch detections are separated by 2.4" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3355369 | 06:27:14.20 +17:29:01.6 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:27:14.20 +17:29:01.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:27:14.20 +17:29:01.6: 12.65 +/- 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
DocumentRef: VOTx3355369,2461274.8960,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3355369 20260822.3960 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.69 05:55:16.95 +25:11:19.0
184.32007 -0.07436 galactic Tau Second-epoch detections are separated by 0.9" and 9.3 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 | DocumentRef: VOTx3366679 | 05:55:16.95 +25:11:19.0 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.788+/-0.026 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:55:16.95 +25:11:19.0: 12.66 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:55:16.95 +25:11:19.0: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 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 08 22.3960* 05 55 16.95 +25 11 19.0 11.7 U Tau 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
DocumentRef: VOTx3366679,2461274.8960,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3366679 20260822.3960 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.51 06:29:55.29 +18:03:16.6
194.44552 3.55438 galactic Gem Second-epoch detections are separated by 4.2" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3371299261483636096 | 06:29:55.13 +18:02:49.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5) J-Ks=1.056+/-0.027 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:55.29 +18:03:16.6: 12.62 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:55.29 +18:03:16.6: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3371299261483636096,2461274.8960,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3371299261483636096 20260822.3960 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.67 06:29:51.51 +17:32:30.5
194.89461 3.30491 galactic Gem Second-epoch detections are separated by 0.6" and 9.8 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 | DocumentRef: VOTx3895391 | 06:29:51.48 +17:32:31.5 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:51.51 +17:32:30.5: 12.67 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:51.51 +17:32:30.5: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 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
DocumentRef: VOTx3895391,2461274.8960,11.67,0.05,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
DocumentRef: VOTx3895391 20260822.3960 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 08 22.3960 2461274.8960 11.77 06:02:07.27 +26:30:14.2
183.94769 1.91529 galactic Gem Second-epoch detections are separated by 2.0" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3429957755850704768 | 06:02:07.28 +26:30:14.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.970+/-0.027 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:02:07.27 +26:30:14.2: 12.66 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:02:07.27 +26:30:14.2: 12.68 +/- 0.03 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
Gaia DR3 3429957755850704768,2461274.8960,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3429957755850704768 20260822.3960 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.74 05:57:37.27 +26:20:53.3
183.58221 0.96358 galactic Tau Second-epoch detections are separated by 1.7" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3429894911890365312 | 05:57:37.21 +26:20:53.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.886+/-0.025 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:57:37.27 +26:20:53.3: 12.66 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:57:37.27 +26:20:53.3: 12.72 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 08 22.3960* 05 57 37.27 +26 20 53.3 11.7 U Tau 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
Gaia DR3 3429894911890365312,2461274.8960,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3429894911890365312 20260822.3960 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.32 06:29:55.17 +18:08:55.2
194.36163 3.59725 galactic Gem Second-epoch detections are separated by 1.4" and 9.9 pix
The object was found in VSX 1" ASASSN-V J062955.21+180855.0
Type: SR
# Max. Min./Amp. JD0 Period
13.930 g Y 0.260 g 2458908.60300 36.490000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:55.17 +18:08:55.2: 12.65 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:55.17 +18:08:55.2: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062955.21+180855.0,2461274.8960,11.32,0.05,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 J062955.21+180855.0 20260822.3960 11.32CV 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 08 22.3960 2461274.8960 11.72 06:02:25.32 +26:46:30.2
183.74479 2.10739 galactic Gem Second-epoch detections are separated by 0.4" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.5999+26.7803 | 06:02:25.30 +26:46:30.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.532+/-0.030 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:02:25.32 +26:46:30.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:02:25.32 +26:46:30.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.5999+26.7803,2461274.8960,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.5999+26.7803 20260822.3960 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 08 22.3960 2461274.8960 11.72 05:55:59.66 +24:59:59.2
184.56439 -0.03032 galactic Tau Second-epoch detections are separated by 1.5" and 9.2 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 | DocumentRef: VOTx3595493 | 05:56:01.24 +25:00:22.8 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE J-Ks=0.176+/-0.035 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:55:59.66 +24:59:59.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:55:59.66 +24:59:59.2: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 08 22.3960* 05 55 59.66 +24 59 59.2 11.7 U Tau 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
DocumentRef: VOTx3595493,2461274.8960,11.72,0.05,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
DocumentRef: VOTx3595493 20260822.3960 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 08 22.3960 2461274.8960 11.72 05:54:25.00 +25:49:07.4
183.67759 0.07538 galactic Tau Second-epoch detections are separated by 3.5" and 9.1 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 | DocumentRef: VOTx3599056 | 05:54:25.00 +25:49:07.4 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.290+/-0.027 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:54:25.00 +25:49:07.4: 12.62 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:54:25.00 +25:49:07.4: 12.81 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 08 22.3960* 05 54 25.00 +25 49 07.4 11.7 U Tau 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
DocumentRef: VOTx3599056,2461274.8960,11.72,0.05,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
DocumentRef: VOTx3599056 20260822.3960 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 08 22.3960 2461274.8960 11.64 06:37:50.88 +18:56:26.2
194.51292 5.63090 galactic Gem Second-epoch detections are separated by 1.5" and 9.7 pix
The object was found in VSX 1" ASASSN-V J063750.84+185626.7
Type: SR
# Max. Min./Amp. JD0 Period
13.830 g Y 0.350 g 2459281.51600 70.650000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:37:50.88 +18:56:26.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:37:50.88 +18:56:26.2: 12.66 +/- 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 J063750.84+185626.7,2461274.8960,11.64,0.05,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 J063750.84+185626.7 20260822.3960 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 08 22.3960 2461274.8960 11.70 05:59:33.61 +26:42:57.4
183.47982 1.52296 galactic Tau Second-epoch detections are separated by 1.8" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3430023554751578752 | 05:59:33.64 +26:42:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.074+/-0.028 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:59:33.61 +26:42:57.4: 12.62 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:59:33.61 +26:42:57.4: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 05 59 33.61 +26 42 57.4 11.7 U Tau 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
Gaia DR3 3430023554751578752,2461274.8960,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3430023554751578752 20260822.3960 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.65 05:55:52.81 +25:12:53.7
184.36550 0.05566 galactic Tau Second-epoch detections are separated by 2.1" and 9.2 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 | 05:55:52.81 +25:12:53.7 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.028 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:55:52.81 +25:12:53.7: 12.64 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:55:52.81 +25:12:53.7: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 05 55 52.81 +25 12 53.7 11.7 U Tau 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,2461274.8960,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3960 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.65 06:32:55.67 +18:36:45.9
194.27606 4.44429 galactic Gem Second-epoch detections are separated by 1.3" and 9.7 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 | 06:32:55.67 +18:36:45.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:32:55.67 +18:36:45.9: 12.60 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:32:55.67 +18:36:45.9: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8960,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3960 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.71 05:58:19.50 +26:06:44.5
183.86536 0.98238 galactic Tau Second-epoch detections are separated by 1.4" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3429839493928833152 | 05:58:19.54 +26:06:44.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.283+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:58:19.50 +26:06:44.5: 12.62 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:58:19.50 +26:06:44.5: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 08 22.3960* 05 58 19.50 +26 06 44.5 11.7 U Tau 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
Gaia DR3 3429839493928833152,2461274.8960,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3429839493928833152 20260822.3960 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 08 22.3960 2461274.8960 11.52 06:25:21.86 +16:59:50.4
194.87996 2.10187 galactic Ori Second-epoch detections are separated by 2.1" and 9.7 pix
The object was found in VSX 1" NSVS J0625217+165949
Type: M
# Max. Min./Amp. JD0 Period
11.900 V < 15.900 V 2451604.00000 443.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:25:21.86 +16:59:50.4: 12.53 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:25:21.86 +16:59:50.4: 13.04 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 06 25 21.86 +16 59 50.4 11.5 U Ori 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 J0625217+165949,2461274.8960,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0625217+165949 20260822.3960 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.62 06:29:01.27 +17:32:32.8
194.80184 3.12811 galactic Gem Second-epoch detections are separated by 1.4" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3369733002870668672 | 06:29:01.28 +17:32:33.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.423+/-0.028 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:01.27 +17:32:32.8: 12.54 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:01.27 +17:32:32.8: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3369733002870668672,2461274.8960,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3369733002870668672 20260822.3960 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.57 06:36:00.55 +19:44:58.9
193.59074 5.60873 galactic Gem Second-epoch detections are separated by 1.1" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3371913716683664768 | 06:36:00.48 +19:44:58.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.300+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:36:00.55 +19:44:58.9: 12.55 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:36:00.55 +19:44:58.9: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3371913716683664768,2461274.8960,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3371913716683664768 20260822.3960 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.62 05:58:26.70 +24:17:05.4
185.46219 0.09298 galactic Tau Second-epoch detections are separated by 1.4" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1147 Stavropolis -386 32 387 17.2 0 0
ATTENTION: measured mag 11.62 is 5.6 mag brighter than the predicted asteroid brightness 17.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:58:26.70 +24:17:05.4: 12.54 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:58:26.70 +24:17:05.4: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 05 58 26.70 +24 17 05.4 11.6 U Tau 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
VARIABLE_NAME,2461274.8960,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260822.3960 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.57 06:36:09.48 +17:08:17.9
195.94376 4.45690 galactic Gem Second-epoch detections are separated by 1.3" and 9.5 pix
The object was found in VSX 1" ASASSN-V J063609.44+170817.7
Type: L
# Max. Min./Amp. JD0 Period
12.940 V 13.040 V
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:36:09.48 +17:08:17.9: 12.53 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:36:09.48 +17:08:17.9: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063609.44+170817.7,2461274.8960,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063609.44+170817.7 20260822.3960 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.65 05:55:26.04 +25:22:14.9
184.18003 0.04711 galactic Tau Second-epoch detections are separated by 1.5" and 9.2 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 | 05:55:26.04 +25:22:14.9 (user input) | T | P | (position from user input) J-Ks=1.185+/-0.043 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:55:26.04 +25:22:14.9: 12.53 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:55:26.04 +25:22:14.9: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 05 55 26.04 +25 22 14.9 11.7 U Tau 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,2461274.8960,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3960 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.59 06:28:38.55 +17:21:56.9
194.91695 2.96642 galactic Gem Second-epoch detections are separated by 2.6" and 10.2 pix
The object was found in VSX19" Gaia DR3 3369694661701875968
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.900 G 14.940 G F
ATTENTION: measured mag 11.59 is 3.3 mag brighter than the VSX record maximum brightness 14.90 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:38.55 +17:21:56.9: 12.54 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:38.55 +17:21:56.9: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3369694661701875968,2461274.8960,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3369694661701875968 20260822.3960 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 10.98 06:28:20.88 +17:32:35.2
194.72700 2.98610 galactic Gem Second-epoch detections are separated by 1.2" and 9.6 pix
The object was found in VSX 1" ASASSN-V J062820.98+173234.8
Type: L
# Max. Min./Amp. JD0 Period
12.630 V 13.130 V
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:20.88 +17:32:35.2: 12.53 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:20.88 +17:32:35.2: 12.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 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 J062820.98+173234.8,2461274.8960,10.98,0.05,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 J062820.98+173234.8 20260822.3960 10.98CV 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 08 22.3960 2461274.8960 11.62 05:57:09.19 +26:25:47.0
183.45908 0.91375 galactic Tau Second-epoch detections are separated by 0.6" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3429906667217046784 | 05:57:09.19 +26:25:48.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.283+/-0.027 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:57:09.19 +26:25:47.0: 12.51 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:57:09.19 +26:25:47.0: 12.72 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 05 57 09.19 +26 25 47.0 11.6 U Tau 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
Gaia DR3 3429906667217046784,2461274.8960,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3429906667217046784 20260822.3960 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.65 05:55:10.80 +26:27:43.6
183.20892 0.54830 galactic Tau Second-epoch detections are separated by 0.9" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.7831+26.4686 | 05:55:10.89 +26:27:43.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.029 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:55:10.80 +26:27:43.6: 12.53 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:55:10.80 +26:27:43.6: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 05 55 10.80 +26 27 43.6 11.7 U Tau 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
ATO J088.7831+26.4686,2461274.8960,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.7831+26.4686 20260822.3960 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.57 06:50:52.56 +22:47:00.8
192.37913 10.05354 galactic Gem Second-epoch detections are separated by 2.5" and 9.9 pix
The object was found in VSX 1" ASASSN-V J065052.53+224659.7
Type: L
# Max. Min./Amp. JD0 Period
13.140 V 13.400 V
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:52.56 +22:47:00.8: 12.49 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:52.56 +22:47:00.8: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J065052.53+224659.7,2461274.8960,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J065052.53+224659.7 20260822.3960 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.24 06:38:06.11 +19:46:27.4
193.79156 6.05941 galactic Gem Second-epoch detections are separated by 1.0" and 9.6 pix
The object was found in VSX 0" ASAS J063806+1946.4
Type: SR|ESD|ED
# Max. Min./Amp. JD0 Period
9.104 Ic Y 0.146 Ic 2452647.80000 109.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:38:06.11 +19:46:27.4: 12.48 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:38:06.11 +19:46:27.4: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 J063806+1946.4,2461274.8960,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J063806+1946.4 20260822.3960 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.49 05:54:54.91 +26:02:58.6
183.53503 0.28880 galactic Tau Second-epoch detections are separated by 2.0" and 9.1 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 | DocumentRef: VOTx3785989 | 05:54:54.91 +26:02:58.6 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:54:54.91 +26:02:58.6: 12.48 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:54:54.91 +26:02:58.6: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 08 22.3960* 05 54 54.91 +26 02 58.6 11.5 U Tau 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
DocumentRef: VOTx3785989,2461274.8960,11.49,0.05,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
DocumentRef: VOTx3785989 20260822.3960 11.49CV 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 08 22.3960 2461274.8960 11.47 06:36:55.38 +19:46:09.2
193.67068 5.80944 galactic Gem Second-epoch detections are separated by 0.7" and 9.7 pix
The object was found in VSX 1" ASASSN-V J063655.42+194609.9
Type: SR
# Max. Min./Amp. JD0 Period
13.520 g Y 0.210 g 2458480.94800 39.040000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:36:55.38 +19:46:09.2: 12.44 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:36:55.38 +19:46:09.2: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063655.42+194609.9,2461274.8960,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063655.42+194609.9 20260822.3960 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.49 06:32:53.53 +18:33:03.0
194.32744 4.40850 galactic Gem Second-epoch detections are separated by 1.1" and 9.6 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 | DocumentRef: VOTx3802271 | 06:32:53.62 +18:33:02.2 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:32:53.53 +18:33:03.0: 12.44 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:32:53.53 +18:33:03.0: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 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
DocumentRef: VOTx3802271,2461274.8960,11.49,0.05,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
DocumentRef: VOTx3802271 20260822.3960 11.49CV 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 08 22.3960 2461274.8960 11.47 06:30:58.14 +19:15:19.1
193.49052 4.32609 galactic Gem Second-epoch detections are separated by 1.6" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.7422+19.2551 | 06:30:58.15 +19:15:18.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:30:58.14 +19:15:19.1: 12.42 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:30:58.14 +19:15:19.1: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.7422+19.2551,2461274.8960,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.7422+19.2551 20260822.3960 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.46 06:26:19.19 +17:29:32.6
194.54762 2.53414 galactic Gem Second-epoch detections are separated by 1.4" and 9.8 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 | DocumentRef: VOTx3822122 | 06:26:19.16 +17:29:33.1 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:26:19.19 +17:29:32.6: 12.41 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:26:19.19 +17:29:32.6: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3822122,2461274.8960,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3822122 20260822.3960 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.39 06:36:51.10 +17:12:47.1
195.95242 4.63847 galactic Gem Second-epoch detections are separated by 1.5" and 9.9 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 | DocumentRef: VOTx3826487 | 06:36:51.03 +17:12:46.8 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=1.220+/-0.028 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:36:51.10 +17:12:47.1: 12.36 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:36:51.10 +17:12:47.1: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 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
DocumentRef: VOTx3826487,2461274.8960,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3826487 20260822.3960 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.39 06:29:39.80 +17:29:57.5
194.91091 3.24404 galactic Gem Second-epoch detections are separated by 2.1" and 10.1 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 | DocumentRef: VOTx3835540 | 06:29:39.80 +17:29:57.5 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.293+/-0.027 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:39.80 +17:29:57.5: 12.33 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:39.80 +17:29:57.5: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3835540,2461274.8960,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3835540 20260822.3960 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.37 05:54:30.35 +25:29:22.8
183.97161 -0.07374 galactic Tau Second-epoch detections are separated by 0.6" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.6201+25.4981 | 05:54:30.36 +25:29:22.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1967AJ.....72.1199M [M67b] +25 42 J-Ks=0.449+/-0.030 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:54:30.35 +25:29:22.8: 12.31 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:54:30.35 +25:29:22.8: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3960* 05 54 30.35 +25 29 22.8 11.4 U Tau 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
ATO J088.6201+25.4981,2461274.8960,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.6201+25.4981 20260822.3960 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.34 06:31:17.51 +19:39:35.3
193.16468 4.57883 galactic Gem Second-epoch detections are separated by 1.7" and 9.7 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 | 06:31:17.51 +19:39:35.3 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=1.115+/-0.033 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:31:17.51 +19:39:35.3: 12.31 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:31:17.51 +19:39:35.3: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8960,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3960 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.36 06:27:30.25 +17:03:49.1
195.05912 2.58559 galactic Gem Second-epoch detections are separated by 1.7" and 9.7 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 | DocumentRef: VOTx3883261 | 06:27:30.25 +17:03:49.1 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.694+/-0.027 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:27:30.25 +17:03:49.1: 12.31 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:27:30.25 +17:03:49.1: 12.35 +/- 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
DocumentRef: VOTx3883261,2461274.8960,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3883261 20260822.3960 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.13 06:28:19.09 +17:13:13.8
195.01010 2.83058 galactic Gem Second-epoch detections are separated by 1.9" and 9.5 pix
The object was found in VSX 1" ASASSN-V J062819.06+171313.2
Type: SR
# Max. Min./Amp. JD0 Period
13.320 g Y 0.240 g 2458377.89400 379.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:19.09 +17:13:13.8: 12.27 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:19.09 +17:13:13.8: 12.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 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 J062819.06+171313.2,2461274.8960,11.13,0.05,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
ASASSN-V J062819.06+171313.2 20260822.3960 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 08 22.3960 2461274.8960 11.29 06:29:53.02 +17:40:06.8
194.78468 3.36863 galactic Gem Second-epoch detections are separated by 1.5" and 9.6 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 | DocumentRef: VOTx3924824 | 06:29:53.04 +17:40:06.4 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE J-Ks=1.027+/-0.037 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:53.02 +17:40:06.8: 12.27 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:53.02 +17:40:06.8: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3924824,2461274.8960,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3924824 20260822.3960 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 12.05 06:39:42.00 +24:25:05.3
189.76288 8.45391 galactic Gem Second-epoch detections are separated by 1.5" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.30 Urania -0 1 1 12.4 0 0
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:39:42.00 +24:25:05.3: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:39:42.00 +24:25:05.3: 15.77 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.77 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461274.8960,12.05,0.05,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
VARIABLE_NAME 20260822.3960 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 08 22.3960 2461274.8960 11.19 06:36:41.66 +18:27:07.7
194.82679 5.16658 galactic Gem Second-epoch detections are separated by 3.1" and 10.3 pix
The object was found in VSX 2" CT Gem
Type: SR
# Max. Min./Amp. JD0 Period
12.790 V Y 0.370 V 2453010.40000 137.808254000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:36:41.66 +18:27:07.7: 12.19 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:36:41.66 +18:27:07.7: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CT Gem,2461274.8960,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CT Gem 20260822.3960 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.26 06:28:55.04 +18:49:51.6
193.64508 3.70052 galactic Gem Second-epoch detections are separated by 1.2" and 9.9 pix
The object was found in VSX 1" ASASSN-V J062855.01+184952.0
Type: SR
# Max. Min./Amp. JD0 Period
12.450 V 12.540 V 2457414.00000 132.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:55.04 +18:49:51.6: 12.14 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:55.04 +18:49:51.6: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062855.01+184952.0,2461274.8960,11.26,0.05,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 J062855.01+184952.0 20260822.3960 11.26CV 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 08 22.3960 2461274.8960 11.19 06:37:41.56 +18:12:13.6
195.15680 5.26562 galactic Gem Second-epoch detections are separated by 1.4" and 10.0 pix
The object was found in VSX 1" ASASSN-V J063741.50+181213.1
Type: SR
# Max. Min./Amp. JD0 Period
12.470 V 12.610 V 2457413.96500 45.370000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:37:41.56 +18:12:13.6: 12.15 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:37:41.56 +18:12:13.6: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 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 J063741.50+181213.1,2461274.8960,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063741.50+181213.1 20260822.3960 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.15 06:29:25.49 +17:51:53.9
194.55964 3.36219 galactic Gem Second-epoch detections are separated by 1.2" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.3562+17.8650 | 06:29:25.51 +17:51:54.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.210+/-0.030 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:25.49 +17:51:53.9: 12.11 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:25.49 +17:51:53.9: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.3562+17.8650,2461274.8960,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.3562+17.8650 20260822.3960 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 11.16 06:34:37.12 +19:54:09.9
193.30502 5.38629 galactic Gem Second-epoch detections are separated by 1.1" and 9.6 pix
The object was found in VSX 1" ASAS J063437+1954.3
Type: MISC
# Max. Min./Amp. JD0 Period
12.350 V Y 0.290 V 2452710.30000 26.200000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:34:37.12 +19:54:09.9: 12.11 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:34:37.12 +19:54:09.9: 12.16 +/- 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 J063437+1954.3,2461274.8960,11.16,0.05,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
ASAS J063437+1954.3 20260822.3960 11.16CV 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 08 22.3960 2461274.8960 11.22 05:56:23.95 +26:00:21.2
183.74077 0.55473 galactic Tau Second-epoch detections are separated by 0.7" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3429858731083449984 | 05:56:23.88 +26:00:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.737+/-0.029 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:56:23.95 +26:00:21.2: 12.12 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:56:23.95 +26:00:21.2: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 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 08 22.3960* 05 56 23.95 +26 00 21.2 11.2 U Tau 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
Gaia DR3 3429858731083449984,2461274.8960,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3429858731083449984 20260822.3960 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 10.93 06:31:14.24 +17:16:37.8
195.28159 3.47517 galactic Gem Second-epoch detections are separated by 1.5" and 9.5 pix
The object was found in VSX 1" ASASSN-V J063114.24+171638.2
Type: SR
# Max. Min./Amp. JD0 Period
12.220 V 12.660 V 2458505.58920 50.253776000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:31:14.24 +17:16:37.8: 12.05 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:31:14.24 +17:16:37.8: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 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 J063114.24+171638.2,2461274.8960,10.93,0.05,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 J063114.24+171638.2 20260822.3960 10.93CV 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 08 22.3960 2461274.8960 11.09 06:28:53.94 +18:23:49.6
194.02888 3.49667 galactic Gem Second-epoch detections are separated by 1.2" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.2247+18.3971 | 06:28:53.94 +18:23:49.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.268+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:53.94 +18:23:49.6: 12.02 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:53.94 +18:23:49.6: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.2247+18.3971,2461274.8960,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.2247+18.3971 20260822.3960 11.09CV 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 08 22.3960 2461274.8960 10.96 06:34:46.40 +17:46:37.2
195.22258 4.45341 galactic Gem Second-epoch detections are separated by 0.8" and 9.9 pix
The object was found in VSX 0" ASAS J063446+1746.7
Type: MISC
# Max. Min./Amp. JD0 Period
12.800 V Y 0.830 V 2453071.20000 204.302780000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:34:46.40 +17:46:37.2: 12.01 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:34:46.40 +17:46:37.2: 12.34 +/- 0.02 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 J063446+1746.7,2461274.8960,10.96,0.05,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
ASAS J063446+1746.7 20260822.3960 10.96CV 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 08 22.3960 2461274.8960 10.95 06:33:31.71 +18:48:11.1
194.17119 4.65766 galactic Gem Second-epoch detections are separated by 0.8" and 9.8 pix
The object was found in VSX 1" ASAS J063332+1848.2
Type: MISC
# Max. Min./Amp. JD0 Period
12.240 V Y 0.450 V 2452794.50000 53.313129000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:33:31.71 +18:48:11.1: 11.95 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:33:31.71 +18:48:11.1: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J063332+1848.2,2461274.8960,10.95,0.05,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
ASAS J063332+1848.2 20260822.3960 10.95CV 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 08 22.3960 2461274.8960 10.80 06:27:55.47 +17:42:06.2
194.53945 2.97001 galactic Gem Second-epoch detections are separated by 0.6" and 9.6 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 | 06:27:55.47 +17:42:06.2 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=1.163+/-0.037 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:27:55.47 +17:42:06.2: 11.73 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:27:55.47 +17:42:06.2: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8960,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3960 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 10.80 06:35:51.44 +17:37:22.5
195.47802 4.61324 galactic Gem Second-epoch detections are separated by 1.3" and 9.9 pix
The object was found in VSX 1" ASASSN-V J063551.48+173721.3
Type: SRS
# Max. Min./Amp. JD0 Period
12.200 V 12.300 V 2457101.79000 20.298000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:35:51.44 +17:37:22.5: 11.78 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:35:51.44 +17:37:22.5: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063551.48+173721.3,2461274.8960,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063551.48+173721.3 20260822.3960 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3960 2461274.8960 10.74 06:29:04.59 +17:52:22.4
194.51432 3.29230 galactic Gem Second-epoch detections are separated by 1.5" and 9.8 pix
The object was found in VSX 0" ASASSN-V J062904.62+175222.6
Type: SR
# Max. Min./Amp. JD0 Period
12.880 g Y 0.130 g 2459225.68700 30.190000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:04.59 +17:52:22.4: 11.71 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:04.59 +17:52:22.4: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 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 J062904.62+175222.6,2461274.8960,10.74,0.05,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 J062904.62+175222.6 20260822.3960 10.74CV 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 08 22.3960 2461274.8960 10.45 06:27:58.00 +17:29:19.8
194.73307 2.88040 galactic Gem Second-epoch detections are separated by 0.5" and 9.8 pix
The object was found in VSX 1" ASASSN-V J062757.99+172918.9
Type: SR
# Max. Min./Amp. JD0 Period
12.600 g Y 0.150 g 2459198.69400 302.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:27:58.00 +17:29:19.8: 11.41 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:27:58.00 +17:29:19.8: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 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 J062757.99+172918.9,2461274.8960,10.45,0.05,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
ASASSN-V J062757.99+172918.9 20260822.3960 10.45CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461274.8960,6.74,0.05,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
VARIABLE_NAME 20260822.3960 6.74CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61760534 18.01.2026 02:49:11.101 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
First image: 2461058.61760534 18.01.2026 02:49:11.101 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Last image: 2461274.89636972 22.08.2026 09:30:36.344 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.79
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 27318
Objects passed selection criteria: 27219
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 16454.5
Average stars matched: 15384.5 (93.4972 %)
Memory usage VmPeak: 252232 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:38:23 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61760534 18.01.2026 02:49:11.101 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
First image: 2461058.61760534 18.01.2026 02:49:11.101 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Last image: 2461274.89636972 22.08.2026 09:30:36.344 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 262
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
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: 25 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): 174542
Objects passed selection criteria: 174037
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 110727
Average stars matched: 106851 (96.4999 %)
Memory usage VmPeak: 642752 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:40:23 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
SExtractor catalog cache: saved Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.cat to cache
SExtractor catalog cache: saved Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.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/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461274.89564535
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_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits exists and is non-empty
wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits exists and is non-empty
wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits (1st reference image)
verification OK: wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:40.095 +22:00:29.68 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits (1st new image)
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:41.584 +22:00:09.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:27:40.095 +22:00:29.68
Second-epoch image center 06:27:41.584 +22:00:09.24
Angular distance between the image centers 0.0081 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits (2nd new image)
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:44.444 +22:00:51.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:27:40.095 +22:00:29.68
Second-epoch image center 06:27:44.444 +22:00:51.42
Angular distance between the image centers 0.0179 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 06:27:41.584 +22:00:09.24
Second-epoch second image center 06:27:44.444 +22:00:51.42
Angular distance between the image centers 0.01610 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/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits &> /tmp/tmp.BXP43pIFa8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.owVs50CD9S
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits &> /tmp/tmp.6sYeplg5Kn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits &> /tmp/tmp.4E3dgAgokX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits and wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits and wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
Found non-empty wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits and wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
The reference image (wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits) and catalog (wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat) found
'wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat' -> 'wcsmag.cat'
Read 29338 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.9455 to 105.5063 deg, Dec +16.3282 to +27.3630 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 87.9455 to 105.5063 deg, Dec 16.3282 to 27.3630 deg
Loaded 19945 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): 14221 out of 15960 total matches.
Matched with Tycho-2 15960 out of 29338 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881900
a=0.000000 b=1.000000 c=22.881900
From vast_summary.log: estimated ref. image limiting mag.: -7.79
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29338 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.9455 to 105.5063 deg, Dec +16.3282 to +27.3630 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 87.9455 to 105.5063 deg, Dec 16.3282 to 27.3630 deg
Loaded 19945 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): 14221 out of 15960 total matches.
Matched with Tycho-2 15960 out of 29338 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Forced-photometry filter: calibrated wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits (aperture=6.2)
Read 31529 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 88.2224 to 105.7491 deg, Dec +16.5172 to +27.2358 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 88.2224 to 105.7491 deg, Dec 16.5172 to 27.2358 deg
Loaded 19341 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): 14457 out of 15956 total matches.
Matched with Tycho-2 15956 out of 31529 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Forced-photometry filter: calibrated wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits -> calib.txt_param_ref_wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
2.5 pix Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
2.7 pix fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
2.6 pix fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
Limiting magnitude estimates:
15.1 mag. Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
15.1 mag. Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
11.7 mag. fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
11.9 mag. fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
All-image limiting magnitude estimate: 11.7 (SNR ) 9.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.BXP43pIFa8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits' -> 'wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Checking if the catalog wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WCS catalog name: wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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=3278, bad_region=0, passed=29338
Got 29338 stars (including 26023 good ones) from the SExtractor catalog wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
util/solve_plate_with_UCAC5 got 29338 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 4818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 29338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 29338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 29338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4819 stars left (next iteration limit 5298)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits N_match=4819 sigma_overall_arcsec=0.370 sigma_q1_arcsec=0.434 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.320 n_q1=1143 n_q2=1240 n_q3=1197 n_q4=1239 worst_quadrant_to_overall_ratio=1.175
The image catalog is written to wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits -region wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.owVs50CD9S (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/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.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_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.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/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat corresponding to the image wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat corresponding to the image wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.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=3030, bad_region=0, passed=31529
Got 31529 stars (including 28473 good ones) from the SExtractor catalog wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat
util/solve_plate_with_UCAC5 got 31529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 4816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 31529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 31529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 31529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 4816 stars left (next iteration limit 5296)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits N_match=4816 sigma_overall_arcsec=0.530 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.684 sigma_q3_arcsec=0.485 sigma_q4_arcsec=0.619 n_q1=1184 n_q2=1326 n_q3=1090 n_q4=1216 worst_quadrant_to_overall_ratio=1.289
The image catalog is written to wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6sYeplg5Kn (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_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.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_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
Checking if the catalog wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
WCS catalog name: wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.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=92, bad_region=0, passed=2658
Got 2658 stars (including 2561 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat
util/solve_plate_with_UCAC5 got 2658 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 2474 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2436 matched stars entering correct_measured_positions(), 2437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2436 matched stars entering correct_measured_positions(), 2657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 2476 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2436 matched stars entering correct_measured_positions(), 2657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 2436 matched stars entering correct_measured_positions(), 2657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 2436 stars left (next iteration limit 2679)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2436 robust_rms=10.418 arcsec worst_quadrant_rms=12.344 arcsec
SIP_REFIT: SIP order 3 trial: matched=2436 robust_rms=0.663 arcsec worst_quadrant_rms=0.807 arcsec
SIP_REFIT: SIP order 5 trial: matched=2436 robust_rms=0.570 arcsec worst_quadrant_rms=0.700 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2436 robust_rms_before=1.535 arcsec robust_rms_before_corrected=0.587 arcsec robust_rms_after=0.570 arcsec worst_quadrant_rms_before=0.647 worst_quadrant_rms_after=0.700
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.647 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits N_match=2436 sigma_overall_arcsec=0.558 sigma_q1_arcsec=0.541 sigma_q2_arcsec=0.648 sigma_q3_arcsec=0.438 sigma_q4_arcsec=0.589 n_q1=530 n_q2=634 n_q3=686 n_q4=586 worst_quadrant_to_overall_ratio=1.162
The image catalog is written to wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits -region wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4E3dgAgokX (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_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.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_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
Checking if the catalog wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
WCS catalog name: wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.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=89, bad_region=0, passed=2700
Got 2700 stars (including 2606 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 2700 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 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 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 2522 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2488 matched stars entering correct_measured_positions(), 2488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2487 matched stars entering correct_measured_positions(), 2699 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 2524 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2488 matched stars entering correct_measured_positions(), 2699 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 2488 matched stars entering correct_measured_positions(), 2699 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 2488 stars left (next iteration limit 2735)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2488 robust_rms=10.207 arcsec worst_quadrant_rms=12.460 arcsec
SIP_REFIT: SIP order 3 trial: matched=2488 robust_rms=0.576 arcsec worst_quadrant_rms=0.695 arcsec
SIP_REFIT: SIP order 5 trial: matched=2488 robust_rms=0.490 arcsec worst_quadrant_rms=0.620 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2488 robust_rms_before=1.542 arcsec robust_rms_before_corrected=0.564 arcsec robust_rms_after=0.490 arcsec worst_quadrant_rms_before=0.623 worst_quadrant_rms_after=0.620
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.623 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits N_match=2488 sigma_overall_arcsec=0.568 sigma_q1_arcsec=0.585 sigma_q2_arcsec=0.625 sigma_q3_arcsec=0.430 sigma_q4_arcsec=0.610 n_q1=529 n_q2=632 n_q3=708 n_q4=619 worst_quadrant_to_overall_ratio=1.099
The image catalog is written to wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits -region wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits to local_wcs_cache/
'wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits' -> 'local_wcs_cache/wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits'
Saving the final (post-refit) wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits'
Saving the final (post-refit) wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits to local_wcs_cache/
'wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits' -> 'local_wcs_cache/wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits'
Saving the final (post-refit) wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits to local_wcs_cache/
'wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits' -> 'local_wcs_cache/wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits sigma_overall=0.370 worst_q_ratio=1.175
ref2=Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits sigma_overall=0.530 worst_q_ratio=1.289
new1=fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits sigma_overall=0.558 worst_q_ratio=1.162
new2=fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits sigma_overall=0.568 worst_q_ratio=1.099
reference average sigma_overall=0.45 worst_q_ratio=1.232
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057_astrometric_residuals.png (4819 matched stars from wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041_astrometric_residuals.png (4816 matched stars from wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130_astrometric_residuals.png (2436 matched stars from wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131_astrometric_residuals.png (2488 matched stars from wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-29-33_20.00sec_-0.00C_LIGHTs_0130.fits'
Saving fully-calibrated image wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Gem-03-Q1b1x1_043158_TTUQ1b1x1_2725819_2hoZrsVJ/wcs_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131.fits'
Preparing the HTML report for the field Gem-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:13:44.33 +22:34:55.6: 14.55 +/- 0.11 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:39.75 +17:18:08.9: 10.61 +/- 0.00 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:37:19.81 +18:12:48.3: 10.30 +/- 0.00 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:13:44.33 +22:34:55.6: 14.36 +/- 0.10 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:39.75 +17:18:08.9: 10.52 +/- 0.00 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:37:19.81 +18:12:48.3: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.08
Forced photometry filter KEPT candidate at 06:13:44.33 +22:34:55.6: ref_mag=14.44 +/- 0.08 new_mean_mag=9.6552 delta=4.79 (need > 0.90)
Forced photometry reference-image weighted average: 10.42 +/- 0.00
Forced photometry reference-image weighted average: 10.56 +/- 0.00
Forced photometry filter KEPT candidate at 06:29:39.75 +17:18:08.9: ref_mag=10.56 +/- 0.00 new_mean_mag=9.6120 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 06:37:19.81 +18:12:48.3: ref_mag=10.42 +/- 0.00 new_mean_mag=9.5074 delta=0.91 (need > 0.90)
Adding exclusion_list_local.txt__out01676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34219.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 55s
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: 2s
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Considering the candidate 34164_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 34164_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:59:22.73 +25:14:09.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 34165_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 34165_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 34219_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 34219_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 16070_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 16070_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:14:52.81 +22:30:21.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 15725_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 15725_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:51:52.68 +22:42:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230761_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 230761_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:58:12.79 +21:57:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230764_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 230764_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:47:04.48 +26:33:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230767_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 230767_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 230768_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 230768_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 230769_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 230769_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:57:51.37 +17:27:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230770_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 230770_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:01:10.53 +23:20:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230771_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 230771_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:22:48.85 +17:48:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230772_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 230772_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:59:22.65 +25:14:08.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 230963_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 230963_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:01:03.58 +23:20:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231113_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 231113_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 231195_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231195_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 231213_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231213_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:29:01.54 +20:10:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231223_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231223_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:58:01.88 +25:55:16.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 231227_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231227_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:03:11.16 +22:21:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231254_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231254_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:14:39.81 +22:29:59.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 231280_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231280_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:14:36.54 +22:29:48.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 231380_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231380_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:01:02.94 +23:18:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231397_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231397_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:49:11.72 +23:13:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231494_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231494_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:01:14.30 +23:18:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231514_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 231514_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:28:51.73 +24:02:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188185_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 188185_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:43:55.80 +25:07:49.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 121764_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 121764_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:22:57.86 +22:30:43.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 32741_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 32741_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 84173_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 84173_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 44719_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 44719_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:32:24.31 +19:07:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203239_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 203239_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:54:59.03 +26:35:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25213_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 25213_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:27:15.39 +18:04:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33134_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 33134_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 158893_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 158893_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:55:37.27 +26:18:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44560_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 44560_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 10645_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 10645_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 17658_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 17658_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:25:18.05 +17:38:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151458_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 151458_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 43817_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 43817_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 158602_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 158602_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 11811_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 11811_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:16:01.06 +17:13:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62558_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 62558_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 218594_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218594_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:46.45 +26:50:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218636_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218636_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:06.73 +26:52:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219045_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219045_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:59.20 +26:51:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219131_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219131_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 219469_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219469_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 219284_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219284_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 219205_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219205_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219083_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219083_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 219067_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219067_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:57.24 +26:53:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219042_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219042_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:02:08.06 +26:56:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219025_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219025_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219019_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219019_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219018_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 219018_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:58:19.60 +26:51:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218885_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218885_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:51.43 +26:52:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218864_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218864_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:55.26 +26:51:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218846_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218846_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 218836_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218836_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:58:05.61 +26:51:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218794_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218794_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:30.23 +26:54:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218776_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218776_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:54:36.99 +26:49:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218772_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218772_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:58:45.87 +26:55:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218733_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218733_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:55:32.64 +26:50:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218729_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218729_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:55:29.72 +26:47:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218697_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218697_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:01:12.73 +26:57:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218626_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 218626_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:58:11.47 +26:54:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29565_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 29565_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:19:43.72 +18:15:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62989_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 62989_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 89941_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 89941_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:37:26.52 +21:22:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59661_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 59661_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:33:58.42 +19:53:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110234_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 110234_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:11.19 +21:51:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31143_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 31143_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 117991_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 117991_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 27378_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 27378_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 42043_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 42043_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 18728_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 18728_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 70632_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 70632_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:45:26.09 +20:28:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08978_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 08978_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 63934_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 63934_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 16417_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 16417_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 27175_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 27175_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 25715_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 25715_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 17572_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 17572_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 57130_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 57130_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 37108_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 37108_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 20546_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 20546_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 27835_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 27835_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 07468_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 07468_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 174133_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 174133_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 42618_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 42618_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 158339_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 158339_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 58686_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 58686_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 17933_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 17933_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:16:17.42 +17:33:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14098_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 14098_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 159305_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 159305_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:55:37.29 +26:16:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180232_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 180232_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 23998_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 23998_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 19035_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 19035_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:37:49.71 +17:50:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14996_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 14996_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 158238_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 158238_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 158716_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 158716_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 25930_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 25930_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 202748_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 202748_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 184093_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 184093_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 167315_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 167315_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 40067_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 40067_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 202883_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 202883_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 180191_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 180191_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171793_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 171793_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:16.42 +25:38:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34292_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 34292_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 163330_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 163330_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:59:26.13 +26:08:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163607_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 163607_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05790_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 05790_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14972_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 14972_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 56382_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 56382_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198986_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 198986_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06761_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 06761_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 176563_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 176563_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43039_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 43039_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:35:30.08 +19:04:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11937_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 11937_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13793_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 13793_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:18:16.11 +17:21:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15380_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 15380_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157646_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 157646_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 157450_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 157450_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20425_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 20425_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:32:33.73 +17:50:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118290_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 118290_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56915_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 56915_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163523_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 163523_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157396_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 157396_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:21.05 +26:24:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56829_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 56829_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 33013_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 33013_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158348_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 158348_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192075_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 192075_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47234_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 47234_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 14583_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 14583_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 08026_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 08026_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 14174_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 14174_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 173912_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 173912_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 55364_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 55364_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06515_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 06515_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 09262_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 09262_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 16996_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 16996_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 163271_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 163271_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:55:07.43 +26:03:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149977_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 149977_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205108_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 205108_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:57:10.53 +26:33:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31367_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 31367_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169391_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 169391_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:54:45.57 +25:43:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161229_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 161229_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:55:07.59 +26:10:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39409_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 39409_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25993_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 25993_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20996_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 20996_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
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Considering the candidate 203441_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 203441_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:17.83 +26:36:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174138_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 174138_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 59937_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 59937_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165106_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 165106_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205777_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 205777_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:55:23.10 +26:27:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183279_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 183279_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10142_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 10142_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161046_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 161046_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:55:12.23 +26:14:05.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30828_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 30828_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18509_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 18509_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38262_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 38262_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18919_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 18919_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15716_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 15716_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21084_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 21084_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159407_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 159407_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:56:26.07 +26:18:40.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14544_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 14544_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11633_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 11633_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:29:39.73 +17:18:08.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118694_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 118694_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:13:44.36 +22:34:55.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136082_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
Preparing report for the candidate 136082_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72726_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 72726_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:28:57.77 +20:12:44.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123712_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 123712_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:14:52.76 +22:30:22.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21350_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 21350_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:32:18.47 +17:46:59.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164731_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 164731_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 05:57:59.78 +25:57:12.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138130_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 138130_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:04:07.43 +23:15:44.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137049_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 137049_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:51:59.92 +23:36:04.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74316_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131
The candidate 74316_fd_Gem-03-Q1b1x1_2026-08-22_04-30-36_20.00sec_0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 06:03:55.30 +20:08:18.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 650s
Prepared the HTML report for the field Gem-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:29:39.75 +17:18:08.9
06:37:19.81 +18:12:48.3
06:13:44.33 +22:34:55.6
06:25:21.86 +16:59:50.4
06:27:30.25 +17:03:49.1
06:36:09.48 +17:08:17.9
06:28:41.22 +17:07:34.2
06:36:51.10 +17:12:47.1
06:28:12.19 +17:12:32.3
06:28:19.09 +17:13:13.8
06:31:14.24 +17:16:37.8
06:28:54.02 +17:18:25.7
06:34:56.99 +22:45:02.8
06:50:52.56 +22:47:00.8
06:28:38.55 +17:21:56.9
06:27:14.20 +17:29:01.6
06:29:39.80 +17:29:57.5
06:27:58.00 +17:29:19.8
06:26:19.19 +17:29:32.6
06:29:01.27 +17:32:32.8
06:29:51.51 +17:32:30.5
06:39:42.00 +24:25:05.3
05:56:31.67 +23:57:33.3
06:28:20.88 +17:32:35.2
06:35:51.44 +17:37:22.5
05:55:10.80 +26:27:43.6
05:57:09.19 +26:25:47.0
06:02:07.27 +26:30:14.2
06:00:27.35 +26:26:03.3
06:01:01.75 +26:26:14.7
05:57:37.27 +26:20:53.3
05:54:54.91 +26:02:58.6
05:58:19.50 +26:06:44.5
06:29:14.49 +17:37:51.4
05:56:23.95 +26:00:21.2
05:54:25.00 +25:49:07.4
06:29:53.02 +17:40:06.8
05:54:30.35 +25:29:22.8
05:56:05.97 +25:30:55.0
06:35:46.76 +17:44:27.1
05:55:26.04 +25:22:14.9
05:55:52.81 +25:12:53.7
05:55:16.95 +25:11:19.0
05:55:59.66 +24:59:59.2
06:34:46.40 +17:46:37.2
06:31:15.57 +17:46:35.4
06:27:55.47 +17:42:06.2
05:58:26.70 +24:17:05.4
06:02:25.32 +26:46:30.2
05:59:33.61 +26:42:57.4
06:29:34.12 +17:51:36.0
06:29:25.49 +17:51:53.9
06:29:04.59 +17:52:22.4
05:58:53.45 +24:23:03.7
06:29:55.29 +18:03:16.6
06:29:05.33 +18:07:42.3
06:29:55.17 +18:08:55.2
06:37:41.56 +18:12:13.6
06:28:24.96 +18:12:14.3
06:29:00.04 +18:13:51.3
06:29:24.20 +18:15:38.7
06:28:53.94 +18:23:49.6
06:20:34.93 +18:19:55.9
06:36:41.66 +18:27:07.7
06:37:01.57 +18:31:41.3
06:32:53.53 +18:33:03.0
06:27:51.95 +18:29:51.4
06:32:55.67 +18:36:45.9
06:38:01.65 +18:48:00.2
06:33:31.71 +18:48:11.1
06:28:55.04 +18:49:51.6
06:37:50.88 +18:56:26.2
06:29:25.55 +18:59:03.0
06:27:43.04 +18:57:36.7
06:32:05.70 +19:05:40.0
06:32:34.66 +19:06:36.0
06:30:58.14 +19:15:19.1
06:31:17.51 +19:39:35.3
06:36:00.55 +19:44:58.9
06:36:55.38 +19:46:09.2
06:38:06.11 +19:46:27.4
06:33:56.06 +19:46:04.3
06:34:19.52 +19:51:36.5
06:34:37.12 +19:54:09.9
06:31:54.44 +20:02:00.3
06:31:50.45 +20:03:28.2
06:32:34.56 +20:06:35.4
06:35:11.51 +21:03:38.5
########### Completed Gem-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:29:59.80 +23:38:52.6
06:13:44.33 +22:34:55.6
06:37:19.81 +18:12:48.3
06:29:39.75 +17:18:08.9
05:58:53.45 +24:23:03.7
06:37:01.57 +18:31:41.3
06:35:11.51 +21:03:38.5
06:27:51.95 +18:29:51.4
06:32:34.66 +19:06:36.0
06:28:54.02 +17:18:25.7
05:56:31.67 +23:57:33.3
06:32:05.70 +19:05:40.0
06:01:01.75 +26:26:14.7
06:31:54.44 +20:02:00.3
06:31:50.45 +20:03:28.2
06:20:34.93 +18:19:55.9
06:34:56.99 +22:45:02.8
06:29:00.04 +18:13:51.3
06:29:25.55 +18:59:03.0
06:31:15.57 +17:46:35.4
06:28:12.19 +17:12:32.3
06:32:34.56 +20:06:35.4
06:29:14.49 +17:37:51.4
06:28:24.96 +18:12:14.3
06:29:05.33 +18:07:42.3
06:35:46.76 +17:44:27.1
06:33:56.06 +19:46:04.3
06:38:01.65 +18:48:00.2
06:29:34.12 +17:51:36.0
06:29:24.20 +18:15:38.7
06:28:41.22 +17:07:34.2
05:56:05.97 +25:30:55.0
06:27:43.04 +18:57:36.7
06:00:27.35 +26:26:03.3
06:34:19.52 +19:51:36.5
06:27:14.20 +17:29:01.6
05:55:16.95 +25:11:19.0
06:29:55.29 +18:03:16.6
06:29:51.51 +17:32:30.5
06:02:07.27 +26:30:14.2
05:57:37.27 +26:20:53.3
06:29:55.17 +18:08:55.2
06:02:25.32 +26:46:30.2
05:55:59.66 +24:59:59.2
05:54:25.00 +25:49:07.4
06:37:50.88 +18:56:26.2
05:59:33.61 +26:42:57.4
05:55:52.81 +25:12:53.7
06:32:55.67 +18:36:45.9
05:58:19.50 +26:06:44.5
06:25:21.86 +16:59:50.4
06:29:01.27 +17:32:32.8
06:36:00.55 +19:44:58.9
05:58:26.70 +24:17:05.4
06:36:09.48 +17:08:17.9
05:55:26.04 +25:22:14.9
06:28:38.55 +17:21:56.9
06:28:20.88 +17:32:35.2
05:57:09.19 +26:25:47.0
05:55:10.80 +26:27:43.6
06:50:52.56 +22:47:00.8
06:38:06.11 +19:46:27.4
05:54:54.91 +26:02:58.6
06:36:55.38 +19:46:09.2
06:32:53.53 +18:33:03.0
06:30:58.14 +19:15:19.1
06:26:19.19 +17:29:32.6
06:36:51.10 +17:12:47.1
06:29:39.80 +17:29:57.5
05:54:30.35 +25:29:22.8
06:31:17.51 +19:39:35.3
06:27:30.25 +17:03:49.1
06:28:19.09 +17:13:13.8
06:29:53.02 +17:40:06.8
06:39:42.00 +24:25:05.3
06:36:41.66 +18:27:07.7
06:28:55.04 +18:49:51.6
06:37:41.56 +18:12:13.6
06:29:25.49 +17:51:53.9
06:34:37.12 +19:54:09.9
05:56:23.95 +26:00:21.2
06:31:14.24 +17:16:37.8
06:28:53.94 +18:23:49.6
06:34:46.40 +17:46:37.2
06:33:31.71 +18:48:11.1
06:27:55.47 +17:42:06.2
06:35:51.44 +17:37:22.5
06:29:04.59 +17:52:22.4
06:27:58.00 +17:29:19.8
06:29:59.90 +23:38:52.8
###################################################################################
06:29:59.80 +23:38:52.6 -- asteroid (will NOT add it to exclusion list)
06:13:44.33 +22:34:55.6 -- asteroid (will NOT add it to exclusion list)
06:37:19.81 +18:12:48.3 -- not an asteroid (will add it to exclusion list)
06:29:39.75 +17:18:08.9 -- not an asteroid (will add it to exclusion list)
05:58:53.45 +24:23:03.7 -- asteroid (will NOT add it to exclusion list)
06:37:01.57 +18:31:41.3 -- not an asteroid (will add it to exclusion list)
06:35:11.51 +21:03:38.5 -- not an asteroid (will add it to exclusion list)
06:27:51.95 +18:29:51.4 -- not an asteroid (will add it to exclusion list)
06:32:34.66 +19:06:36.0 -- not an asteroid (will add it to exclusion list)
06:28:54.02 +17:18:25.7 -- not an asteroid (will add it to exclusion list)
05:56:31.67 +23:57:33.3 -- not an asteroid (will add it to exclusion list)
06:32:05.70 +19:05:40.0 -- not an asteroid (will add it to exclusion list)
06:01:01.75 +26:26:14.7 -- not an asteroid (will add it to exclusion list)
06:31:54.44 +20:02:00.3 -- not an asteroid (will add it to exclusion list)
06:31:50.45 +20:03:28.2 -- not an asteroid (will add it to exclusion list)
06:20:34.93 +18:19:55.9 -- not an asteroid (will add it to exclusion list)
06:34:56.99 +22:45:02.8 -- asteroid (will NOT add it to exclusion list)
06:29:00.04 +18:13:51.3 -- not an asteroid (will add it to exclusion list)
06:29:25.55 +18:59:03.0 -- not an asteroid (will add it to exclusion list)
06:31:15.57 +17:46:35.4 -- not an asteroid (will add it to exclusion list)
06:28:12.19 +17:12:32.3 -- not an asteroid (will add it to exclusion list)
06:32:34.56 +20:06:35.4 -- not an asteroid (will add it to exclusion list)
06:29:14.49 +17:37:51.4 -- not an asteroid (will add it to exclusion list)
06:28:24.96 +18:12:14.3 -- not an asteroid (will add it to exclusion list)
06:29:05.33 +18:07:42.3 -- not an asteroid (will add it to exclusion list)
06:35:46.76 +17:44:27.1 -- not an asteroid (will add it to exclusion list)
06:33:56.06 +19:46:04.3 -- not an asteroid (will add it to exclusion list)
06:38:01.65 +18:48:00.2 -- not an asteroid (will add it to exclusion list)
06:29:34.12 +17:51:36.0 -- not an asteroid (will add it to exclusion list)
06:29:24.20 +18:15:38.7 -- not an asteroid (will add it to exclusion list)
06:28:41.22 +17:07:34.2 -- not an asteroid (will add it to exclusion list)
05:56:05.97 +25:30:55.0 -- not an asteroid (will add it to exclusion list)
06:27:43.04 +18:57:36.7 -- not an asteroid (will add it to exclusion list)
06:00:27.35 +26:26:03.3 -- not an asteroid (will add it to exclusion list)
06:34:19.52 +19:51:36.5 -- not an asteroid (will add it to exclusion list)
06:27:14.20 +17:29:01.6 -- not an asteroid (will add it to exclusion list)
05:55:16.95 +25:11:19.0 -- not an asteroid (will add it to exclusion list)
06:29:55.29 +18:03:16.6 -- not an asteroid (will add it to exclusion list)
06:29:51.51 +17:32:30.5 -- not an asteroid (will add it to exclusion list)
06:02:07.27 +26:30:14.2 -- not an asteroid (will add it to exclusion list)
05:57:37.27 +26:20:53.3 -- not an asteroid (will add it to exclusion list)
06:29:55.17 +18:08:55.2 -- not an asteroid (will add it to exclusion list)
06:02:25.32 +26:46:30.2 -- not an asteroid (will add it to exclusion list)
05:55:59.66 +24:59:59.2 -- not an asteroid (will add it to exclusion list)
05:54:25.00 +25:49:07.4 -- not an asteroid (will add it to exclusion list)
06:37:50.88 +18:56:26.2 -- not an asteroid (will add it to exclusion list)
05:59:33.61 +26:42:57.4 -- not an asteroid (will add it to exclusion list)
05:55:52.81 +25:12:53.7 -- not an asteroid (will add it to exclusion list)
06:32:55.67 +18:36:45.9 -- not an asteroid (will add it to exclusion list)
05:58:19.50 +26:06:44.5 -- not an asteroid (will add it to exclusion list)
06:25:21.86 +16:59:50.4 -- not an asteroid (will add it to exclusion list)
06:29:01.27 +17:32:32.8 -- not an asteroid (will add it to exclusion list)
06:36:00.55 +19:44:58.9 -- not an asteroid (will add it to exclusion list)
05:58:26.70 +24:17:05.4 -- asteroid (will NOT add it to exclusion list)
06:36:09.48 +17:08:17.9 -- not an asteroid (will add it to exclusion list)
05:55:26.04 +25:22:14.9 -- not an asteroid (will add it to exclusion list)
06:28:38.55 +17:21:56.9 -- not an asteroid (will add it to exclusion list)
06:28:20.88 +17:32:35.2 -- not an asteroid (will add it to exclusion list)
05:57:09.19 +26:25:47.0 -- not an asteroid (will add it to exclusion list)
05:55:10.80 +26:27:43.6 -- not an asteroid (will add it to exclusion list)
06:50:52.56 +22:47:00.8 -- not an asteroid (will add it to exclusion list)
06:38:06.11 +19:46:27.4 -- not an asteroid (will add it to exclusion list)
05:54:54.91 +26:02:58.6 -- not an asteroid (will add it to exclusion list)
06:36:55.38 +19:46:09.2 -- not an asteroid (will add it to exclusion list)
06:32:53.53 +18:33:03.0 -- not an asteroid (will add it to exclusion list)
06:30:58.14 +19:15:19.1 -- not an asteroid (will add it to exclusion list)
06:26:19.19 +17:29:32.6 -- not an asteroid (will add it to exclusion list)
06:36:51.10 +17:12:47.1 -- not an asteroid (will add it to exclusion list)
06:29:39.80 +17:29:57.5 -- not an asteroid (will add it to exclusion list)
05:54:30.35 +25:29:22.8 -- not an asteroid (will add it to exclusion list)
06:31:17.51 +19:39:35.3 -- not an asteroid (will add it to exclusion list)
06:27:30.25 +17:03:49.1 -- not an asteroid (will add it to exclusion list)
06:28:19.09 +17:13:13.8 -- not an asteroid (will add it to exclusion list)
06:29:53.02 +17:40:06.8 -- not an asteroid (will add it to exclusion list)
06:39:42.00 +24:25:05.3 -- asteroid (will NOT add it to exclusion list)
06:36:41.66 +18:27:07.7 -- not an asteroid (will add it to exclusion list)
06:28:55.04 +18:49:51.6 -- not an asteroid (will add it to exclusion list)
06:37:41.56 +18:12:13.6 -- not an asteroid (will add it to exclusion list)
06:29:25.49 +17:51:53.9 -- not an asteroid (will add it to exclusion list)
06:34:37.12 +19:54:09.9 -- not an asteroid (will add it to exclusion list)
05:56:23.95 +26:00:21.2 -- not an asteroid (will add it to exclusion list)
06:31:14.24 +17:16:37.8 -- not an asteroid (will add it to exclusion list)
06:28:53.94 +18:23:49.6 -- not an asteroid (will add it to exclusion list)
06:34:46.40 +17:46:37.2 -- not an asteroid (will add it to exclusion list)
06:33:31.71 +18:48:11.1 -- not an asteroid (will add it to exclusion list)
06:27:55.47 +17:42:06.2 -- not an asteroid (will add it to exclusion list)
06:35:51.44 +17:37:22.5 -- not an asteroid (will add it to exclusion list)
06:29:04.59 +17:52:22.4 -- not an asteroid (will add it to exclusion list)
06:27:58.00 +17:29:19.8 -- not an asteroid (will add it to exclusion list)
06:29:59.90 +23:38:52.8 -- asteroid (will NOT add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:54:25.00 +25:49:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:30.35 +25:29:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:54.91 +26:02:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:10.80 +26:27:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:16.95 +25:11:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:26.04 +25:22:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:52.81 +25:12:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:59.66 +24:59:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:05.97 +25:30:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:23.95 +26:00:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:31.67 +23:57:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:09.19 +26:25:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:37.27 +26:20:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:19.50 +26:06:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:33.61 +26:42:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:27.35 +26:26:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:01.75 +26:26:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:07.27 +26:30:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:25.32 +26:46:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:34.93 +18:19:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:21.86 +16:59:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.19 +17:29:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:14.20 +17:29:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:30.25 +17:03:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:43.04 +18:57:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:51.95 +18:29:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:55.47 +17:42:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:58.00 +17:29:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:12.19 +17:12:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:19.09 +17:13:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:20.88 +17:32:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:24.96 +18:12:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:38.55 +17:21:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:41.22 +17:07:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:53.94 +18:23:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:54.02 +17:18:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:55.04 +18:49:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:00.04 +18:13:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:01.27 +17:32:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:04.59 +17:52:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:05.33 +18:07:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:14.49 +17:37:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:24.20 +18:15:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:25.49 +17:51:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:25.55 +18:59:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:34.12 +17:51:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:39.75 +17:18:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:39.80 +17:29:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:51.51 +17:32:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:53.02 +17:40:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:55.17 +18:08:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:55.29 +18:03:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:58.14 +19:15:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:14.24 +17:16:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:15.57 +17:46:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:17.51 +19:39:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:50.45 +20:03:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:54.44 +20:02:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:05.70 +19:05:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:34.56 +20:06:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:34.66 +19:06:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:53.53 +18:33:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:55.67 +18:36:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:31.71 +18:48:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:56.06 +19:46:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:19.52 +19:51:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:37.12 +19:54:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:46.40 +17:46:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:11.51 +21:03:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:46.76 +17:44:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:51.44 +17:37:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:00.55 +19:44:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:09.48 +17:08:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:41.66 +18:27:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:51.10 +17:12:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:55.38 +19:46:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:01.57 +18:31:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:19.81 +18:12:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:41.56 +18:12:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:50.88 +18:56:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:01.65 +18:48:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:06.11 +19:46:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:52.56 +22:47:00.8 -- 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)
05:54:25.00 +25:49:07.4 -- not a known variable star
05:54:30.35 +25:29:22.8 -- not a known variable star
05:54:54.91 +26:02:58.6 -- not a known variable star
05:55:10.80 +26:27:43.6 -- not a known variable star
05:55:16.95 +25:11:19.0 -- not a known variable star
05:55:26.04 +25:22:14.9 -- not a known variable star
05:55:52.81 +25:12:53.7 -- not a known variable star
05:55:59.66 +24:59:59.2 -- not a known variable star
05:56:05.97 +25:30:55.0 -- not a known variable star
05:56:23.95 +26:00:21.2 -- not a known variable star
05:56:31.67 +23:57:33.3 -- not a known variable star
05:57:09.19 +26:25:47.0 -- not a known variable star
05:57:37.27 +26:20:53.3 -- not a known variable star
05:58:19.50 +26:06:44.5 -- not a known variable star
05:59:33.61 +26:42:57.4 -- not a known variable star
06:00:27.35 +26:26:03.3 -- not a known variable star
06:01:01.75 +26:26:14.7 -- not a known variable star
06:02:07.27 +26:30:14.2 -- not a known variable star
06:02:25.32 +26:46:30.2 -- not a known variable star
06:20:34.93 +18:19:55.9 -- a known variable star
06:25:21.86 +16:59:50.4 -- a known variable star
06:26:19.19 +17:29:32.6 -- not a known variable star
06:27:14.20 +17:29:01.6 -- not a known variable star
06:27:30.25 +17:03:49.1 -- not a known variable star
06:27:43.04 +18:57:36.7 -- a known variable star
06:27:51.95 +18:29:51.4 -- a known variable star
06:27:55.47 +17:42:06.2 -- not a known variable star
06:27:58.00 +17:29:19.8 -- a known variable star
06:28:12.19 +17:12:32.3 -- not a known variable star
06:28:19.09 +17:13:13.8 -- a known variable star
06:28:20.88 +17:32:35.2 -- a known variable star
06:28:24.96 +18:12:14.3 -- not a known variable star
06:28:38.55 +17:21:56.9 -- a known variable star
06:28:41.22 +17:07:34.2 -- not a known variable star
06:28:53.94 +18:23:49.6 -- not a known variable star
06:28:54.02 +17:18:25.7 -- not a known variable star
06:28:55.04 +18:49:51.6 -- a known variable star
06:29:00.04 +18:13:51.3 -- not a known variable star
06:29:01.27 +17:32:32.8 -- not a known variable star
06:29:04.59 +17:52:22.4 -- a known variable star
06:29:05.33 +18:07:42.3 -- not a known variable star
06:29:14.49 +17:37:51.4 -- not a known variable star
06:29:24.20 +18:15:38.7 -- not a known variable star
06:29:25.49 +17:51:53.9 -- not a known variable star
06:29:25.55 +18:59:03.0 -- not a known variable star
06:29:34.12 +17:51:36.0 -- not a known variable star
06:29:39.75 +17:18:08.9 -- a known variable star
06:29:39.80 +17:29:57.5 -- not a known variable star
06:29:51.51 +17:32:30.5 -- not a known variable star
06:29:53.02 +17:40:06.8 -- not a known variable star
06:29:55.17 +18:08:55.2 -- a known variable star
06:29:55.29 +18:03:16.6 -- not a known variable star
06:30:58.14 +19:15:19.1 -- not a known variable star
06:31:14.24 +17:16:37.8 -- a known variable star
06:31:15.57 +17:46:35.4 -- not a known variable star
06:31:17.51 +19:39:35.3 -- not a known variable star
06:31:50.45 +20:03:28.2 -- not a known variable star
06:31:54.44 +20:02:00.3 -- a known variable star
06:32:05.70 +19:05:40.0 -- not a known variable star
06:32:34.56 +20:06:35.4 -- not a known variable star
06:32:34.66 +19:06:36.0 -- not a known variable star
06:32:53.53 +18:33:03.0 -- not a known variable star
06:32:55.67 +18:36:45.9 -- not a known variable star
06:33:31.71 +18:48:11.1 -- a known variable star
06:33:56.06 +19:46:04.3 -- a known variable star
06:34:19.52 +19:51:36.5 -- not a known variable star
06:34:37.12 +19:54:09.9 -- a known variable star
06:34:46.40 +17:46:37.2 -- a known variable star
06:35:11.51 +21:03:38.5 -- a known variable star
06:35:46.76 +17:44:27.1 -- a known variable star
06:35:51.44 +17:37:22.5 -- a known variable star
06:36:00.55 +19:44:58.9 -- not a known variable star
06:36:09.48 +17:08:17.9 -- a known variable star
06:36:41.66 +18:27:07.7 -- a known variable star
06:36:51.10 +17:12:47.1 -- not a known variable star
06:36:55.38 +19:46:09.2 -- a known variable star
06:37:01.57 +18:31:41.3 -- a known variable star
06:37:19.81 +18:12:48.3 -- a known variable star
06:37:41.56 +18:12:13.6 -- a known variable star
06:37:50.88 +18:56:26.2 -- a known variable star
06:38:01.65 +18:48:00.2 -- a known variable star
06:38:06.11 +19:46:27.4 -- a known variable star
06:50:52.56 +22:47:00.8 -- a known variable star
Found 52 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
83 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 83 (excluding asteroids and hot pixels, 52 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)2461274.89564535 -observatory V36
09:45:31.89 +15:17:26.5 Mercury (-1.7mag)
12:50:20.20 -07:47:42.0 Venus (-4.5mag)
06:29:58.88 +23:38:57.0 Mars (1.3mag)
08:55:32.08 +17:52:55.9 Jupiter (-1.8mag)
00:54:48.86 +03:01:29.5 Saturn (0.5mag)
04:13:02.42 +21:00:19.7 Uranus (5.7mag)
00:15:07.82 +00:06:15.2 Neptune (7.7mag)
20:26:50.41 -23:35:12.8 Pluto (14.5mag)
17:29:17.33 -28:25:40.0 Moon (-11.0mag)
-rw-r--r-- 1 apache apache 363 Aug 22 04:38 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461274.89564535:
08:55:34.92 +17:52:42.8 Io (6.1mag)
08:55:40.00 +17:52:20.0 Europa (6.3mag)
08:55:48.38 +17:51:41.6 Ganymede (5.6mag)
08:55:12.97 +17:54:25.7 Callisto (6.9mag)
08:53:00.32 +18:00:57.7 Himalia (15.7mag)
08:55:30.39 +17:53:04.3 Thebe (16.6mag)
08:52:39.57 +17:56:49.5 Elara (17.7mag)
08:59:39.66 +17:26:10.2 Pasiphae (17.9mag)
08:57:45.03 +18:06:31.5 Carme (19.0mag)
00:54:45.05 +03:01:54.9 Titan (8.4mag)
00:54:53.43 +03:01:21.1 Rhea (9.7mag)
00:55:24.32 +03:03:10.8 Iapetus (11.1mag)
00:54:56.55 +03:01:46.5 Hyperion (14.4mag)
00:53:53.58 +02:52:54.6 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 22 04:38 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461274.89564535:
20:12:00.96 -14:01:16.0 JWST
17:38:08.29 +34:11:51.2 Chandra
11:32:30.02 -60:44:50.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 22 04:38 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461274.89564535 -observatory V36
03:28:17.42 +18:26:38.1 17.5mag P/1996 R2 (Lagerkvist)
17:59:54.66 -34:28:32.8 14.2mag P/2010 H2 (Vales)
07:06:32.35 -69:29:31.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:13:09.09 +33:18:30.5 17.7mag C/2017 K2 (PANSTARRS)
04:21:12.18 +42:25:06.5 17.5mag P/2021 N1 (ZTF)
22:26:41.87 +30:22:27.3 17.4mag C/2022 E2 (ATLAS)
06:56:56.82 +26:16:58.0 16.8mag C/2022 N2 (PANSTARRS)
10:34:44.65 +27:51:01.5 17.0mag C/2022 QE78 (ATLAS)
09:38:19.75 +05:17:59.2 18.0mag C/2022 R6 (PANSTARRS)
15:15:40.58 -12:52:47.9 18.0mag P/2023 B1 (PANSTARRS)
20:53:23.41 +64:03:52.6 18.0mag C/2023 H5 (Lemmon)
15:36:27.49 -14:14:11.6 14.6mag C/2023 R1 (PANSTARRS)
08:23:17.97 +32:00:52.4 15.5mag C/2024 E1 (Wierzchos)
15:05:42.19 +15:30:14.8 17.8mag C/2024 G6 (ATLAS)
18:46:49.02 +43:29:22.8 13.7mag C/2024 J3 (ATLAS)
20:49:21.05 +49:41:19.4 17.5mag C/2024 R4 (PANSTARRS)
05:25:47.33 -12:53:57.9 15.3mag C/2024 T5 (ATLAS)
07:04:37.90 +21:36:01.0 17.9mag C/2025 J1 (Borisov)
10:53:19.60 +19:57:18.6 17.1mag C/2025 V2 (Rankin)
13:07:25.38 +01:21:05.1 16.9mag C/2025 Y1 (ATLAS)
16:10:32.55 +76:17:05.5 16.5mag C/2026 A2 (Bok)
03:09:55.48 +46:20:59.6 17.3mag C/2026 B2 (Sun-Gao)
11:58:53.29 +09:55:53.1 17.4mag A/2026 E1
22:12:26.17 -32:18:46.2 7.1mag 10P/Tempel
11:37:44.77 -04:19:23.7 16.3mag 29P/Schwassmann-Wachmann
11:36:29.37 +00:00:42.0 17.4mag 63P/Wild
00:51:36.79 -06:06:17.1 15.4mag 65P/Gunn
06:06:51.79 +20:14:28.5 13.7mag 78P/Gehrels
20:25:48.07 -25:00:10.3 17.5mag 84P/Giclas
03:12:01.06 +14:32:20.3 16.9mag 88P/Howell
08:30:35.67 +25:34:49.8 16.4mag 93P/Lovas
04:47:41.02 +22:25:40.9 17.2mag 112P/Urata-Niijima
06:42:41.10 +28:17:28.1 16.1mag 114P/Wiseman-Skiff
09:51:44.32 +24:05:13.1 14.9mag 123P/West-Hartley
12:12:35.93 -15:37:09.3 17.3mag 124P/Mrkos
05:56:48.24 +21:01:43.3 16.0mag 128P/Shoemaker-Holt
06:52:00.65 +18:05:54.6 17.9mag 131P/Mueller
23:59:36.66 +03:05:57.3 17.4mag 139P/Vaisala-Oterma
03:09:34.52 -18:37:30.3 12.8mag 161P/Hartley-IRAS
08:03:44.20 +38:07:18.0 16.1mag 162P/Siding Spring
11:03:47.67 +29:52:47.5 12.2mag 169P/NEAT
03:06:13.93 +09:23:35.9 17.6mag 220P/McNaught
20:16:20.20 -51:48:17.6 18.0mag 259P/Garradd
04:03:22.63 +30:50:36.5 15.3mag 260P/McNaught
07:47:24.79 +37:05:09.0 17.3mag 295P/LINEAR
15:16:12.33 +01:33:02.0 17.8mag 391P/Kowalski
09:13:44.95 +17:39:57.3 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.3K Aug 22 04:38 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
-rw-r--r-- 1 apache apache 5.7K Aug 22 04:38 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
-rw-r--r-- 1 apache apache 190K Aug 22 04:38 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:27:30.457 +02:47:32.36 AT 2026xfu 2026-01-14.53 21.69
17:59:19.284 +29:24:54.02 AT 2026xft 2026-07-18.43 20.84
19:54:12.936 -24:01:35.76 AT 2026xfs 2026-05-17.56 19.77
08:44:08.771 +29:07:45.05 AT 2026xfr 2026-01-14.38 20.4
23:28:59.311 -21:41:17.71 AT 2026xfq 2026-07-19.57 21.15
20:34:55.430 -31:12:10.98 AT 2026xfp 2026-07-14.44 20
13:01:30.092 +38:12:35.50 AT 2026xfo 2026-06-23.28 20.85
23:22:05.758 +18:57:29.94 AT 2026xfn 2026-07-25.52 21.28
10:13:35.246 -20:37:42.73 AT 2026xfm 2026-01-27.58 21
21:57:25.287 +03:48:20.98 AT 2026xfl 2026-07-16.55 21.68
14:26:07.382 +33:39:52.18 AT 2026xfk 2026-06-13.34 20.9
02:09:31.559 -03:10:04.80 AT 2026xfj 2026-01-17.24 21.98
20:17:01.562 -20:06:27.94 AT 2026xfi 2026-05-20.56 20.93
21:08:09.912 -21:12:24.85 AT 2026xfh 2026-06-19.58 20.9
20:08:20.135 -25:53:36.34 AT 2026xfg 2026-07-19.45 20.74
14:51:25.078 +41:07:07.07 AT 2026xff 2026-06-13.34 21.62
22:33:15.210 +12:04:33.49 AT 2026xfe 2026-06-21.53 20.23
13:52:05.795 +29:21:47.19 AT 2026xfd 2026-04-24.32 20.92
13:30:27.613 +10:38:39.93 AT 2026xfc 2026-04-20.32 21.07
13:40:18.442 +39:30:10.71 AT 2026xfb 2026-05-24.29 20.6
-rw-r--r-- 1 apache apache 87K Aug 22 04:38 tns_transients_list.txt
