This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 9.51 06:41:56.99 +22:56:10.9
191.33713 8.26654 galactic Gem Second-epoch detections are separated by 0.9" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1 Ceres -0 -0 0 8.8 -0 -0
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:41:56.99 +22:56:10.9: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:41:56.99 +22:56:10.9: 15.67 +/- 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,2461293.9826,9.51,0.05,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
VARIABLE_NAME 20260910.4826 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 09 10.4826 2461293.9826 11.31 06:30:33.02 +17:37:45.1
194.89293 3.49151 galactic Gem Second-epoch detections are separated by 1.3" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3369725821687893376 | 06:30:32.93 +17:37:44.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.150+/-0.030 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:30:33.02 +17:37:45.1: 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 06:30:33.02 +17:37:45.1: 12.17 +/- 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
Gaia DR3 3369725821687893376,2461293.9826,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3369725821687893376 20260910.4826 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.16 06:45:22.09 +26:47:35.0
188.15071 10.63232 galactic Gem Second-epoch detections are separated by 0.5" and 9.6 pix
The object was found in VSX22" ZTF J064521.68+264756.3
Type: EW
# Max. Min./Amp. JD0 Period
18.634 r Y 0.274 r 2458357.01220 0.260219400000
ATTENTION: measured mag 11.16 is 7.2 mag brighter than the VSX record maximum brightness 18.36 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:22.09 +26:47:35.0: 12.22 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:22.09 +26:47:35.0: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J064521.68+264756.3,2461293.9826,11.16,0.05,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
ZTF J064521.68+264756.3 20260910.4826 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 09 10.4826 2461293.9826 11.12 06:43:38.13 +26:23:38.1
188.34963 10.11169 galactic Gem Second-epoch detections are separated by 0.3" 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 J100.9088+26.3938 | 06:43:38.13 +26:23:38.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=1.085+/-0.023 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:38.13 +26:23:38.1: 12.28 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:38.13 +26:23:38.1: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 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 J100.9088+26.3938,2461293.9826,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9088+26.3938 20260910.4826 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.37 06:50:13.15 +24:34:30.4
190.66618 10.68055 galactic Gem Second-epoch detections are separated by 2.0" 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 3381405349593349376 | 06:50:13.13 +24:34:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.746+/-0.026 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:13.15 +24:34:30.4: 12.30 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:13.15 +24:34:30.4: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3381405349593349376,2461293.9826,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3381405349593349376 20260910.4826 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.39 06:43:57.72 +26:27:28.2
188.32275 10.20511 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 | Gaia DR3 3384951549468880128 | 06:43:57.72 +26:27:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5) J-Ks=0.220+/-0.033 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:57.72 +26:27:28.2: 12.40 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:57.72 +26:27:28.2: 12.36 +/- 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
Gaia DR3 3384951549468880128,2461293.9826,11.39,0.05,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
Gaia DR3 3384951549468880128 20260910.4826 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 09 10.4826 2461293.9826 11.76 06:42:45.60 +26:29:33.8
188.17359 9.97707 galactic Gem Second-epoch detections are separated by 2.0" 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 | target | 06:42:45.60 +26:29:33.8 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.190+/-0.030 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:45.60 +26:29:33.8: 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 06:42:45.60 +26:29:33.8: 12.65 +/- 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
target,2461293.9826,11.76,0.05,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
target 20260910.4826 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 09 10.4826 2461293.9826 11.69 06:50:34.73 +24:31:49.1
190.74276 10.73564 galactic Gem Second-epoch detections are separated by 2.6" 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 | target | 06:50:34.73 +24:31:49.1 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.406+/-0.027 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:34.73 +24:31:49.1: 12.88 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:34.73 +24:31:49.1: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.98 06:43:41.16 +26:18:40.2
188.43049 10.08644 galactic Gem Second-epoch detections are separated by 6.2" and 10.6 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 J100.9205+26.3004 | 06:43:41.16 +26:18:40.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=0.644+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:41.16 +26:18:40.2: 13.43 +/- 0.04 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:41.16 +26:18:40.2: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9205+26.3004,2461293.9826,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9205+26.3004 20260910.4826 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.91 06:45:38.84 +26:32:11.7
188.41387 10.57975 galactic Gem Second-epoch detections are separated by 1.3" 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 | target | 06:45:38.84 +26:32:11.7 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.564+/-0.027 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:38.84 +26:32:11.7: 13.20 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:38.84 +26:32:11.7: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 12.01 06:44:18.25 +26:39:57.8
188.16467 10.36328 galactic Gem Second-epoch detections are separated by 3.4" and 9.0 pix
The object was found in VSX 1" EPIC 202066941
Type: E
# Max. Min./Amp. JD0 Period
13.100 Kp Y 0.120 Kp 0.605169000000
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 06:44:18.25 +26:39:57.8: 13.21 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:18.25 +26:39:57.8: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 202066941,2461293.9826,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 202066941 20260910.4826 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.77 06:44:28.54 +26:43:03.1
188.13395 10.41989 galactic Gem Second-epoch detections are separated by 0.5" 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 | 06:44:28.54 +26:43:03.1 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.254+/-0.028 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:28.54 +26:43:03.1: 13.14 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:28.54 +26:43:03.1: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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,2461293.9826,11.77,0.05,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
target 20260910.4826 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.68 06:50:19.25 +24:26:30.7
190.79896 10.64499 galactic Gem 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 | ATO J102.5660+24.4433 | 06:50:19.25 +24:26:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.527+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:19.25 +24:26:30.7: 13.11 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:19.25 +24:26:30.7: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5660+24.4433,2461293.9826,11.68,0.05,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
ATO J102.5660+24.4433 20260910.4826 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 09 10.4826 2461293.9826 11.87 06:44:20.98 +26:42:03.1
188.13708 10.38733 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 | ATO J101.0853+26.7001 | 06:44:20.98 +26:42:03.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G9 (LAMOST DR5)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:20.98 +26:42:03.1: 13.10 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:20.98 +26:42:03.1: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.0853+26.7001,2461293.9826,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.0853+26.7001 20260910.4826 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.94 06:42:34.25 +26:01:49.1
188.57873 9.73979 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 | target | 06:42:34.25 +26:01:49.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.430+/-0.035 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:34.25 +26:01:49.1: 13.05 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:42:34.25 +26:01:49.1: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.65 06:45:03.16 +26:39:24.5
188.24567 10.51061 galactic Gem Second-epoch detections are separated by 1.7" 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 | 06:45:03.16 +26:39:24.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.750+/-0.026 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:03.16 +26:39:24.5: 13.03 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:03.16 +26:39:24.5: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.65,0.05,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 20260910.4826 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.79 06:44:11.54 +26:27:18.7
188.34758 10.25058 galactic Gem Second-epoch detections are separated by 1.7" 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 | target | 06:44:11.54 +26:27:18.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.785+/-0.031 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:11.54 +26:27:18.7: 13.02 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:11.54 +26:27:18.7: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.92 06:43:30.33 +26:01:09.7
188.68047 9.92461 galactic Gem Second-epoch detections are separated by 1.6" 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 | target | 06:43:30.33 +26:01:09.7 (user input) | T | P | (position from user input) J-Ks=0.492+/-0.029 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:30.33 +26:01:09.7: 12.98 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:30.33 +26:01:09.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.84 06:44:25.21 +26:43:45.6
188.11772 10.41371 galactic Gem Second-epoch detections are separated by 2.6" 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 J101.1049+26.7261 | 06:44:25.21 +26:43:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.380+/-0.027 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:25.21 +26:43:45.6: 12.92 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:25.21 +26:43:45.6: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1049+26.7261,2461293.9826,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.1049+26.7261 20260910.4826 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.67 06:44:34.96 +26:43:05.9
188.14360 10.44183 galactic Gem Second-epoch detections are separated by 1.0" and 9.8 pix
The object was found in VSX 0" EPIC 202068346
Type: VAR
# Max. Min./Amp. JD0 Period
10.600 Kp Y 0.005 Kp
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 06:44:34.96 +26:43:05.9: 12.89 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:34.96 +26:43:05.9: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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
EPIC 202068346,2461293.9826,11.67,0.05,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
EPIC 202068346 20260910.4826 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 09 10.4826 2461293.9826 11.85 06:42:59.49 +26:33:39.8
188.13350 10.05317 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 | target | 06:42:59.49 +26:33:39.8 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.564+/-0.033 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:59.49 +26:33:39.8: 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 06:42:59.49 +26:33:39.8: 12.85 +/- 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
target,2461293.9826,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.74 06:43:43.87 +26:22:04.9
188.38271 10.11995 galactic Gem Second-epoch detections are separated by 0.7" 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 | Gaia DR3 3384948560171646976 | 06:43:43.90 +26:22:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.869+/-0.031 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:43.87 +26:22:04.9: 12.88 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:43.87 +26:22:04.9: 12.77 +/- 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
Gaia DR3 3384948560171646976,2461293.9826,11.74,0.05,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 3384948560171646976 20260910.4826 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.91 06:43:58.25 +25:50:50.4
188.88381 9.94518 galactic Gem Second-epoch detections are separated by 0.5" 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 | target | 06:43:58.25 +25:50:50.4 (user input) | T | P | (position from user input) J-Ks=0.216+/-0.033 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:58.25 +25:50:50.4: 12.86 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:58.25 +25:50:50.4: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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,2461293.9826,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.80 06:52:57.89 +25:53:56.7
189.70731 11.80034 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 | 06:52:57.89 +25:53:56.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.784+/-0.029 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:52:57.89 +25:53:56.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:52:57.89 +25:53:56.7: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.69 06:44:43.83 +26:50:07.4
188.05017 10.52157 galactic Gem Second-epoch detections are separated by 2.5" 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 | target | 06:44:43.83 +26:50:07.4 (user input) | T | P | (position from user input) J-Ks=0.639+/-0.026 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:43.83 +26:50:07.4: 12.81 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:43.83 +26:50:07.4: 12.73 +/- 0.02 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
target,2461293.9826,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.59 06:44:54.87 +26:33:17.4
188.32611 10.43922 galactic Gem Second-epoch detections are separated by 1.0" 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 | 06:44:54.87 +26:33:17.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.232+/-0.030 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:54.87 +26:33:17.4: 12.80 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:54.87 +26:33:17.4: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.59,0.05,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
target 20260910.4826 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 09 10.4826 2461293.9826 11.63 06:43:12.87 +26:20:56.8
188.34965 10.00729 galactic Gem Second-epoch detections are separated by 2.3" 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 | target | 06:43:12.87 +26:20:56.8 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.306+/-0.026 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:12.87 +26:20:56.8: 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 06:43:12.87 +26:20:56.8: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 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,2461293.9826,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.53 06:45:24.94 +26:47:57.2
188.14962 10.64454 galactic Gem Second-epoch detections are separated by 0.0" and 9.7 pix
The object was found in VSX 1" Gaia DR3 3384986772498346112
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.710 G 12.740 G A
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 06:45:24.94 +26:47:57.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:24.94 +26:47:57.2: 12.78 +/- 0.02 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
Gaia DR3 3384986772498346112,2461293.9826,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384986772498346112 20260910.4826 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.62 06:50:46.92 +24:31:05.2
190.77393 10.77234 galactic Gem Second-epoch detections are separated by 0.6" 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 | 06:50:46.92 +24:31:05.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.338+/-0.027 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:46.92 +24:31:05.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:46.92 +24:31:05.2: 12.78 +/- 0.02 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
target,2461293.9826,11.62,0.05,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
target 20260910.4826 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.80 06:42:46.54 +26:09:14.8
188.48545 9.83462 galactic Gem Second-epoch detections are separated by 1.0" 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 | 06:42:46.54 +26:09:14.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.259+/-0.032 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:46.54 +26:09:14.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:42:46.54 +26:09:14.8: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.59 06:50:44.85 +24:24:02.2
190.87888 10.71546 galactic Gem 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 | Gaia DR3 3381210396733026944 | 06:50:47.29 +24:23:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.265+/-0.028 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:44.85 +24:24:02.2: 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 06:50:44.85 +24:24:02.2: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 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 3381210396733026944,2461293.9826,11.59,0.05,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 3381210396733026944 20260910.4826 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 09 10.4826 2461293.9826 11.74 06:52:49.23 +25:44:37.8
189.83764 11.70612 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 | target | 06:52:49.23 +25:44:37.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.542+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:52:49.23 +25:44:37.8: 12.68 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:52:49.23 +25:44:37.8: 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9826,11.74,0.05,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
target 20260910.4826 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.69 06:45:03.04 +24:57:03.1
189.81178 9.78007 galactic Gem Second-epoch detections are separated by 0.9" 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 | 06:45:03.04 +24:57:03.1 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.133+/-0.029 (A)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:03.04 +24:57:03.1: 12.68 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:03.04 +24:57:03.1: 12.63 +/- 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
target,2461293.9826,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4826 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.51 06:43:29.10 +26:16:20.6
188.44644 10.02911 galactic Gem Second-epoch detections are separated by 1.5" 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 | 06:43:29.10 +26:16:20.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.415+/-0.025 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:29.10 +26:16:20.6: 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 06:43:29.10 +26:16:20.6: 12.62 +/- 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
target,2461293.9826,11.51,0.05,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
target 20260910.4826 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.56 06:45:54.55 +26:43:57.4
188.25858 10.71599 galactic Gem Second-epoch detections are separated by 1.8" 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 J101.4771+26.7323 | 06:45:54.55 +26:43:57.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.758+/-0.039 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:54.55 +26:43:57.4: 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 06:45:54.55 +26:43:57.4: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.4771+26.7323,2461293.9826,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.4771+26.7323 20260910.4826 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.52 06:45:42.09 +26:35:21.6
188.37053 10.61314 galactic Gem Second-epoch detections are separated by 3.3" 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 3384932239296950528 | 06:45:42.07 +26:35:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.700+/-0.026 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:42.09 +26:35:21.6: 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 06:45:42.09 +26:35:21.6: 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
Gaia DR3 3384932239296950528,2461293.9826,11.52,0.05,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
Gaia DR3 3384932239296950528 20260910.4826 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 09 10.4826 2461293.9826 11.73 05:55:15.56 +23:08:05.0
186.09096 -1.11496 galactic Tau Second-epoch detections are separated by 1.5" and 10.4 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 3424781942302253696 | 05:55:15.44 +23:08:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.807+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:55:15.56 +23:08:05.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:55:15.56 +23:08:05.0: 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 09 10.4826* 05 55 15.56 +23 08 05.0 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 3424781942302253696,2461293.9826,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3424781942302253696 20260910.4826 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.66 06:50:48.92 +24:43:26.8
190.58716 10.86636 galactic Gem Second-epoch detections are separated by 0.9" 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 | target | 06:50:48.92 +24:43:26.8 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.209+/-0.028 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:48.92 +24:43:26.8: 12.63 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:48.92 +24:43:26.8: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 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,2461293.9826,11.66,0.05,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
target 20260910.4826 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.66 06:50:07.69 +24:33:03.9
190.67940 10.65163 galactic Gem Second-epoch detections are separated by 2.4" 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 | ATO J102.5341+24.5464 | 06:50:07.75 +24:33:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.654+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:07.69 +24:33:03.9: 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 06:50:07.69 +24:33:03.9: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5341+24.5464,2461293.9826,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.5341+24.5464 20260910.4826 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.61 06:44:51.09 +25:08:04.9
189.62367 9.81840 galactic Gem Second-epoch detections are separated by 1.9" 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 3384486902726958208 | 06:44:51.07 +25:08:05.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.254+/-0.030 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:51.09 +25:08:04.9: 12.59 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:51.09 +25:08:04.9: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 3384486902726958208,2461293.9826,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384486902726958208 20260910.4826 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.44 06:50:41.53 +24:29:53.3
190.78353 10.74537 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 3381216164873194112 | 06:50:41.55 +24:29:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.847+/-0.027 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:41.53 +24:29:53.3: 12.57 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:41.53 +24:29:53.3: 12.61 +/- 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
Gaia DR3 3381216164873194112,2461293.9826,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3381216164873194112 20260910.4826 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.62 05:54:39.64 +22:54:46.3
186.21301 -1.34585 galactic Tau Second-epoch detections are separated by 4.1" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J055437.08+225442.1 | 05:54:37.08 +22:54:42.1 (Gaia DR3) | SR (local) | 336.000000000000 (local) | Gaia3var=NOT_AVAILABLE 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 05:54:39.64 +22:54:46.3: 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 05:54:39.64 +22:54:46.3: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 09 10.4826* 05 54 39.64 +22 54 46.3 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
ASASSN-V J055437.08+225442.1,2461293.9826,11.62,0.05,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
ASASSN-V J055437.08+225442.1 20260910.4826 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.39 06:43:14.40 +26:26:50.7
188.26197 10.05463 galactic Gem Second-epoch detections are separated by 1.0" and 9.7 pix
The object was found in VSX22" Gaia DR3 3384953752789970688
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.700 G 13.740 G F
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 06:43:14.40 +26:26:50.7: 12.50 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:14.40 +26:26:50.7: 12.42 +/- 0.01 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
Gaia DR3 3384953752789970688,2461293.9826,11.39,0.05,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
Gaia DR3 3384953752789970688 20260910.4826 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 09 10.4826 2461293.9826 11.54 06:47:42.89 +24:46:00.1
190.24373 10.24719 galactic Gem Second-epoch detections are separated by 0.2" 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 | Gaia DR3 3381469434802054912 | 06:47:42.92 +24:46:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F4 (LAMOST DR5) J-Ks=0.293+/-0.028 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:47:42.89 +24:46:00.1: 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 06:47:42.89 +24:46:00.1: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 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 3381469434802054912,2461293.9826,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3381469434802054912 20260910.4826 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.43 06:50:24.43 +24:33:13.6
190.70429 10.71023 galactic Gem Second-epoch detections are separated by 0.9" and 9.6 pix
The object was found in VSX 1" ASASSN-V J065024.46+243312.9
Type: EA
# Max. Min./Amp. JD0 Period
12.500 V 12.660 V 2458003.10000 86.350000000000
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 06:50:24.43 +24:33:13.6: 12.45 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:24.43 +24:33:13.6: 12.44 +/- 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
ASASSN-V J065024.46+243312.9,2461293.9826,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J065024.46+243312.9 20260910.4826 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.44 06:43:59.02 +26:35:24.6
188.20330 10.26610 galactic Gem Second-epoch detections are separated by 2.2" 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 3384961341995347968 | 06:43:59.02 +26:35:24.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.629+/-0.030 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:59.02 +26:35:24.6: 12.43 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:59.02 +26:35:24.6: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 3384961341995347968,2461293.9826,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384961341995347968 20260910.4826 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.43 06:43:36.27 +26:21:39.5
188.37684 10.09129 galactic Gem Second-epoch detections are separated by 0.9" 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 3384948598829217536 | 06:43:36.26 +26:21:39.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.308+/-0.026 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:36.27 +26:21:39.5: 12.40 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:36.27 +26:21:39.5: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 3384948598829217536,2461293.9826,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384948598829217536 20260910.4826 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.21 06:44:41.48 +26:43:40.8
188.14520 10.46791 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 | ATO J101.1728+26.7279 | 06:44:41.49 +26:43:40.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.924+/-0.024 (M)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:41.48 +26:43:40.8: 12.36 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:41.48 +26:43:40.8: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1728+26.7279,2461293.9826,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.1728+26.7279 20260910.4826 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.46 06:43:13.07 +26:30:12.1
188.20848 10.07415 galactic Gem Second-epoch detections are separated by 1.6" 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 | ATO J100.7953+26.4958 | 06:43:13.08 +26:30:12.0 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.534+/-0.027 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:13.07 +26:30:12.1: 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 06:43:13.07 +26:30:12.1: 12.31 +/- 0.01 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
ATO J100.7953+26.4958,2461293.9826,11.46,0.05,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
ATO J100.7953+26.4958 20260910.4826 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 09 10.4826 2461293.9826 11.23 06:45:08.01 +26:47:40.0
188.12678 10.58551 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 3384986665122511232 | 06:45:08.07 +26:47:40.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.352+/-0.028 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:08.01 +26:47:40.0: 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 06:45:08.01 +26:47:40.0: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3384986665122511232,2461293.9826,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384986665122511232 20260910.4826 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.38 06:43:23.03 +26:11:48.4
188.50590 9.97616 galactic Gem Second-epoch detections are separated by 0.4" 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 3384806177713894656 | 06:43:23.04 +26:11:47.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.747+/-0.026 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:23.03 +26:11:48.4: 12.36 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:23.03 +26:11:48.4: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 3384806177713894656,2461293.9826,11.38,0.05,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
Gaia DR3 3384806177713894656 20260910.4826 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.46 06:52:51.37 +25:48:00.9
189.78868 11.73694 galactic Gem Second-epoch detections are separated by 1.2" and 9.5 pix
The object was found in VSX 0" EPIC 202086754
Type: VAR
# Max. Min./Amp. JD0 Period
12.400 Kp Y 0.002 Kp 6.964525000000
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 06:52:51.37 +25:48:00.9: 12.35 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:52:51.37 +25:48:00.9: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.32 +/- 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
EPIC 202086754,2461293.9826,11.46,0.05,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
EPIC 202086754 20260910.4826 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 09 10.4826 2461293.9826 11.47 06:44:07.91 +26:10:19.2
188.60173 10.11712 galactic Gem Second-epoch detections are separated by 0.8" 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 3384896058491409024 | 06:44:07.98 +26:10:18.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.393+/-0.031 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:07.91 +26:10:19.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:07.91 +26:10:19.2: 12.32 +/- 0.01 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
Gaia DR3 3384896058491409024,2461293.9826,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384896058491409024 20260910.4826 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.37 06:50:15.26 +24:32:23.2
190.70220 10.67281 galactic Gem Second-epoch detections are separated by 0.7" 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 | ATO J102.5597+24.5523 | 06:50:15.27 +24:32:23.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.296+/-0.028 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:15.26 +24:32:23.2: 12.35 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:15.26 +24:32:23.2: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5597+24.5523,2461293.9826,11.37,0.05,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 J102.5597+24.5523 20260910.4826 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.34 06:52:11.06 +25:59:20.2
189.54919 11.67830 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 | ATO J103.0452+25.9909 | 06:52:11.06 +25:59:20.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:52:11.06 +25:59:20.2: 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 06:52:11.06 +25:59:20.2: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 J103.0452+25.9909,2461293.9826,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0452+25.9909 20260910.4826 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.29 06:44:39.24 +26:48:27.6
188.06829 10.49432 galactic Gem Second-epoch detections are separated by 0.7" 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 | Gaia DR3 3384989035944457984 | 06:44:39.26 +26:48:27.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.720+/-0.028 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:39.24 +26:48:27.6: 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 06:44:39.24 +26:48:27.6: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3384989035944457984,2461293.9826,11.29,0.05,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
Gaia DR3 3384989035944457984 20260910.4826 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.27 06:42:51.29 +26:12:31.3
188.44320 9.87414 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 | Gaia DR3 3384852662143550976 | 06:42:51.29 +26:12:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.318+/-0.029 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:51.29 +26:12:31.3: 12.30 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:42:51.29 +26:12:31.3: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3384852662143550976,2461293.9826,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384852662143550976 20260910.4826 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.38 06:51:47.29 +25:56:04.4
189.56168 11.57468 galactic Gem Second-epoch detections are separated by 0.9" 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 J102.9366+25.9309 | 06:51:47.29 +25:56:04.8 (Gaia DR3) | DBF (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.596+/-0.025 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:51:47.29 +25:56:04.4: 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 06:51:47.29 +25:56:04.4: 12.25 +/- 0.01 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
ATO J102.9366+25.9309,2461293.9826,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9366+25.9309 20260910.4826 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.27 06:45:54.80 +26:39:00.7
188.33493 10.68185 galactic Gem Second-epoch detections are separated by 1.3" 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 3384934300881248768 | 06:45:54.78 +26:39:00.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.361+/-0.027 (G)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:54.80 +26:39:00.7: 12.29 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:54.80 +26:39:00.7: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 3384934300881248768,2461293.9826,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384934300881248768 20260910.4826 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.10 06:45:35.73 +26:43:48.2
188.23068 10.65149 galactic Gem Second-epoch detections are separated by 0.7" 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 3384938630208276096 | 06:45:35.80 +26:43:48.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=0.628+/-0.027 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:35.73 +26:43:48.2: 12.28 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:35.73 +26:43:48.2: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3384938630208276096,2461293.9826,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384938630208276096 20260910.4826 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.31 06:31:20.75 +17:59:17.3
194.66060 3.82458 galactic Gem Second-epoch detections are separated by 1.0" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1251 Hedera -15 -341 341 16.2 0 0
ATTENTION: measured mag 11.31 is 4.9 mag brighter than the predicted asteroid brightness 16.2 - 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 06:31:20.75 +17:59:17.3: 12.28 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:31:20.75 +17:59:17.3: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461293.9826,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260910.4826 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.39 06:31:23.27 +17:58:05.5
194.68296 3.82431 galactic Gem Second-epoch detections are separated by 0.2" and 10.2 pix
The object was found in VSX 0" Gaia DR3 3371242563615862272
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.050 G 12.090 G F
The object was found in astcheck.1251 Hedera 21 -413 413 16.2 0 0
NOTE: the measured brightness disagrees with the predicted asteroid brightness, but the matched variable star above likely accounts for this object.
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:31:23.27 +17:58:05.5: 12.23 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:31:23.27 +17:58:05.5: 12.28 +/- 0.01 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
Gaia DR3 3371242563615862272,2461293.9826,11.39,0.05,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
Gaia DR3 3371242563615862272 20260910.4826 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 09 10.4826 2461293.9826 11.29 06:44:54.82 +24:48:01.7
189.93594 9.68729 galactic Gem Second-epoch detections are separated by 1.0" 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 | Gaia DR3 3384460312588064512 | 06:44:54.81 +24:48:02.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.271+/-0.028 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:54.82 +24:48:01.7: 12.23 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:54.82 +24:48:01.7: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 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 3384460312588064512,2461293.9826,11.29,0.05,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
Gaia DR3 3384460312588064512 20260910.4826 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.33 06:30:53.56 +17:51:47.8
194.72217 3.67150 galactic Gem Second-epoch detections are separated by 1.3" 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 | ATO J097.7125+17.8718 | 06:30:51.92 +17:52:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.203+/-0.029 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:30:53.56 +17:51:47.8: 12.20 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:30:53.56 +17:51:47.8: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 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 J097.7125+17.8718,2461293.9826,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.7125+17.8718 20260910.4826 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.20 06:40:53.36 +26:14:29.8
188.22008 9.49073 galactic Gem Second-epoch detections are separated by 0.9" and 9.9 pix
The object was found in VSX 1" ASASSN-V J064053.37+261429.0
Type: L
# Max. Min./Amp. JD0 Period
12.100 V 12.470 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 06:40:53.36 +26:14:29.8: 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 06:40:53.36 +26:14:29.8: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 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 J064053.37+261429.0,2461293.9826,11.20,0.05,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 J064053.37+261429.0 20260910.4826 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 09 10.4826 2461293.9826 11.25 06:44:33.54 +24:52:49.3
189.82764 9.64910 galactic Gem Second-epoch detections are separated by 1.5" 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 J101.1368+24.8770 | 06:44:33.52 +24:52:49.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5) J-Ks=0.074+/-0.028 (A)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:33.54 +24:52:49.3: 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 06:44:33.54 +24:52:49.3: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1368+24.8770,2461293.9826,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.1368+24.8770 20260910.4826 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.05 06:43:26.81 +26:23:07.7
188.33898 10.06990 galactic Gem Second-epoch detections are separated by 0.9" 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 | Gaia DR3 3384949247366412672 | 06:43:26.82 +26:23:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.309+/-0.025 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:26.81 +26:23:07.7: 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 06:43:26.81 +26:23:07.7: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3384949247366412672,2461293.9826,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384949247366412672 20260910.4826 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 11.02 06:46:07.18 +26:43:09.0
188.29127 10.75285 galactic Gem Second-epoch detections are separated by 2.0" 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 3384943337492433664 | 06:46:07.17 +26:43:08.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.622+/-0.027 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:46:07.18 +26:43:09.0: 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 06:46:07.18 +26:43:09.0: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3384943337492433664,2461293.9826,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384943337492433664 20260910.4826 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 10.96 06:50:50.12 +24:32:14.5
190.76140 10.79148 galactic Gem Second-epoch detections are separated by 1.1" 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 | Gaia DR3 3381216714629007232 | 06:50:50.12 +24:32:14.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.597+/-0.027 (K)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:50.12 +24:32:14.5: 11.88 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:50.12 +24:32:14.5: 11.94 +/- 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
Gaia DR3 3381216714629007232,2461293.9826,10.96,0.05,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
Gaia DR3 3381216714629007232 20260910.4826 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 09 10.4826 2461293.9826 10.79 06:45:12.16 +26:46:16.2
188.15490 10.58958 galactic Gem Second-epoch detections are separated by 0.5" 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 | ATO J101.2988+26.7667 | 06:45:12.17 +26:46:16.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.246+/-0.026 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:12.16 +26:46:16.2: 11.79 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:12.16 +26:46:16.2: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.2988+26.7667,2461293.9826,10.79,0.05,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 J101.2988+26.7667 20260910.4826 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 10.65 06:45:17.77 +26:43:58.2
188.19922 10.59217 galactic Gem Second-epoch detections are separated by 0.6" and 9.8 pix
The object was found in VSX 0" EPIC 202072712
Type: VAR
# Max. Min./Amp. JD0 Period
11.600 Kp Y 0.005 Kp
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 06:45:17.77 +26:43:58.2: 11.64 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:17.77 +26:43:58.2: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 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
EPIC 202072712,2461293.9826,10.65,0.05,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
EPIC 202072712 20260910.4826 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4826 2461293.9826 10.62 06:44:53.71 +26:47:04.9
188.11274 10.53323 galactic Gem Second-epoch detections are separated by 0.4" 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 3384988078168436224 | 06:44:53.73 +26:47:05.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.283+/-0.026 (F)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:53.71 +26:47:04.9: 11.55 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:53.71 +26:47:04.9: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 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 3384988078168436224,2461293.9826,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3384988078168436224 20260910.4826 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461293.98293763 10.09.2026 11:35:15.811 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
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): 27262
Objects passed selection criteria: 27163
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 15888.5
Average stars matched: 14833.2 (93.3584 %)
Memory usage VmPeak: 252236 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Sep 10 02:28:55 CDT 2026
VaST build number 1.0rc89-204-g1bee8b93
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 10 06:38:30 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: 2461293.98293763 10.09.2026 11:35:15.811 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 110
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: 24 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): 174231
Objects passed selection criteria: 173701
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: 106183
Average stars matched: 102380 (96.4182 %)
Memory usage VmPeak: 577216 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Sep 10 02:28:55 CDT 2026
VaST build number 1.0rc89-204-g1bee8b93
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 10 06:39:45 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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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: 2461293.98226567
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_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits exists and is non-empty
wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits (1st new image)
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:45.134 +22:00:01.01 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 06:27:45.134 +22:00:01.01
Angular distance between the image centers 0.0210 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits (2nd new image)
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:48.181 +21:59:19.24 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 06:27:48.181 +21:59:19.24
Angular distance between the image centers 0.0369 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 06:27:45.134 +22:00:01.01
Second-epoch second image center 06:27:48.181 +21:59:19.24
Angular distance between the image centers 0.01653 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.nYgQVLXdRz
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.bpur90kqYA
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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits &> /tmp/tmp.cV61S69ilD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits &> /tmp/tmp.3q1yduLSaN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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 1 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
2.9 pix fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
2.9 pix fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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
11.4 mag. fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
11.9 mag. fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
All-image limiting magnitude estimate: 11.4 (SNR ) 9.6 (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.nYgQVLXdRz (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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.bpur90kqYA (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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.cV61S69ilD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
Checking if the catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.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_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
WCS catalog name: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.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=63, bad_region=0, passed=1435
Got 1435 stars (including 1371 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat
util/solve_plate_with_UCAC5 got 1435 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 589 (Dec 16.5 to 27.4)
Done reading UCAC5 zone files...
Matched 1304 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1275 matched stars entering correct_measured_positions(), 1248 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1275 matched stars entering correct_measured_positions(), 1401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 589 (Dec 16.5 to 27.4)
Done reading UCAC5 zone files...
Matched 1305 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1271 matched stars entering correct_measured_positions(), 1401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 1271 matched stars entering correct_measured_positions(), 1401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 1271 stars left (next iteration limit 1402)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1271 robust_rms=14.915 arcsec worst_quadrant_rms=17.727 arcsec
SIP_REFIT: SIP order 3 trial: matched=1271 robust_rms=0.560 arcsec worst_quadrant_rms=0.645 arcsec
SIP_REFIT: SIP order 5 trial: matched=1271 robust_rms=0.432 arcsec worst_quadrant_rms=0.574 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1271 robust_rms_before=0.918 arcsec robust_rms_before_corrected=0.638 arcsec robust_rms_after=0.432 arcsec worst_quadrant_rms_before=0.968 worst_quadrant_rms_after=0.574
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:45.132 +22:00:00.37 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1435 stars ###
'wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/correct_sextractor_wcs_catalog_usingxy2sky3762783.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.918 -> 0.432 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 1271 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 589 (Dec 16.5 to 27.4)
Done reading UCAC5 zone files...
Matched 1194 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 1194 pairs (1271 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=1194 robust_rms=14.624 arcsec worst_quadrant_rms=17.547 arcsec
SIP_REFIT: SIP order 3 trial: matched=1194 robust_rms=0.547 arcsec worst_quadrant_rms=0.650 arcsec
SIP_REFIT: SIP order 5 trial: matched=1194 robust_rms=0.427 arcsec worst_quadrant_rms=0.564 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1194 robust_rms_before=0.428 arcsec robust_rms_before_corrected=0.428 arcsec robust_rms_after=0.427 arcsec worst_quadrant_rms_before=0.553 worst_quadrant_rms_after=0.564
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.564 vs 0.553 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 1194 matched stars entering correct_measured_positions(), 1399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 1194 matched stars entering correct_measured_positions(), 1398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
WCS_QUALITY_DIAG: file=fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits N_match=1194 sigma_overall_arcsec=0.436 sigma_q1_arcsec=0.455 sigma_q2_arcsec=0.539 sigma_q3_arcsec=0.401 sigma_q4_arcsec=0.408 n_q1=293 n_q2=207 n_q3=332 n_q4=362 worst_quadrant_to_overall_ratio=1.236
The image catalog is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits -region wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.3q1yduLSaN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
Checking if the catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
WCS catalog name: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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=81, bad_region=0, passed=1638
Got 1638 stars (including 1552 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat
util/solve_plate_with_UCAC5 got 1638 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 27.4)
Done reading UCAC5 zone files...
Matched 1477 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1449 matched stars entering correct_measured_positions(), 1416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1449 matched stars entering correct_measured_positions(), 1597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 27.4)
Done reading UCAC5 zone files...
Matched 1478 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1451 matched stars entering correct_measured_positions(), 1597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 1451 matched stars entering correct_measured_positions(), 1597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 1451 stars left (next iteration limit 1593)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1451 robust_rms=12.874 arcsec worst_quadrant_rms=15.712 arcsec
SIP_REFIT: SIP order 3 trial: matched=1451 robust_rms=0.509 arcsec worst_quadrant_rms=0.618 arcsec
SIP_REFIT: SIP order 5 trial: matched=1451 robust_rms=0.381 arcsec worst_quadrant_rms=0.473 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1451 robust_rms_before=0.868 arcsec robust_rms_before_corrected=0.576 arcsec robust_rms_after=0.381 arcsec worst_quadrant_rms_before=0.747 worst_quadrant_rms_after=0.473
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:48.172 +21:59:18.51 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1638 stars ###
'wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/correct_sextractor_wcs_catalog_usingxy2sky3762834.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.868 -> 0.381 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 1451 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 1375 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 1375 pairs (1451 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=1375 robust_rms=12.512 arcsec worst_quadrant_rms=14.926 arcsec
SIP_REFIT: SIP order 3 trial: matched=1375 robust_rms=0.498 arcsec worst_quadrant_rms=0.590 arcsec
SIP_REFIT: SIP order 5 trial: matched=1375 robust_rms=0.377 arcsec worst_quadrant_rms=0.458 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1375 robust_rms_before=0.378 arcsec robust_rms_before_corrected=0.378 arcsec robust_rms_after=0.377 arcsec worst_quadrant_rms_before=0.459 worst_quadrant_rms_after=0.458
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:48.172 +21:59:18.52 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1638 stars ###
'wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/correct_sextractor_wcs_catalog_usingxy2sky3763800.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.378 -> 0.377 arcsec)
Accuracy estimation diagnostic: 1375 matched stars entering correct_measured_positions(), 1598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 1375 matched stars entering correct_measured_positions(), 1596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WCS_QUALITY_DIAG: file=fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits N_match=1375 sigma_overall_arcsec=0.395 sigma_q1_arcsec=0.456 sigma_q2_arcsec=0.487 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.374 n_q1=333 n_q2=183 n_q3=384 n_q4=475 worst_quadrant_to_overall_ratio=1.234
The image catalog is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits -region wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_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_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits to local_wcs_cache/
'wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits' -> 'local_wcs_cache/wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits'
Saving the final (post-refit) wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits to local_wcs_cache/
'wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits' -> 'local_wcs_cache/wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits sigma_overall=0.436 worst_q_ratio=1.236
new2=fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits sigma_overall=0.395 worst_q_ratio=1.234
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_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093_astrometric_residuals.png (1194 matched stars from wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094_astrometric_residuals.png (1375 matched stars from wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits'
Saving fully-calibrated image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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 06:41:56.99 +22:56:10.9: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:41:56.99 +22:56:10.9: 15.67 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out34184.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34184_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 34184_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Gem-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:41:56.99 +22:56:10.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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_vSTL
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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Creating symlink local_wcs_cache/wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
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
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_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits exists and is non-empty
wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits (1st new image)
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:45.132 +22:00:00.37 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 06:27:45.132 +22:00:00.37
Angular distance between the image centers 0.0211 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits (2nd new image)
verification OK: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:48.172 +21:59:18.52 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 06:27:48.172 +21:59:18.52
Angular distance between the image centers 0.0369 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 06:27:45.132 +22:00:00.37
Second-epoch second image center 06:27:48.172 +21:59:18.52
Angular distance between the image centers 0.01653 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.0YvLAdgjaO
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.fxD2PsAR8A
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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits &> /tmp/tmp.jvk8afUUEQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits &> /tmp/tmp.3U5K1oOBBT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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 206292 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.9318 to 105.5265 deg, Dec +16.3091 to +27.3656 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 87.9318 to 105.5265 deg, Dec 16.3091 to 27.3656 deg
Loaded 20018 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): 11191 out of 16872 total matches.
Matched with Tycho-2 16872 out of 206292 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.736100
a=0.000000 b=1.000000 c=22.736100
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.27
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.27
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 206292 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.9318 to 105.5265 deg, Dec +16.3091 to +27.3656 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 87.9318 to 105.5265 deg, Dec 16.3091 to 27.3656 deg
Loaded 20018 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): 11191 out of 16872 total matches.
Matched with Tycho-2 16872 out of 206292 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=4.7)
Read 188638 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 88.2221 to 105.7490 deg, Dec +16.4980 to +27.2397 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 88.2221 to 105.7490 deg, Dec 16.4980 to 27.2397 deg
Loaded 19379 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): 11515 out of 16583 total matches.
Matched with Tycho-2 16583 out of 188638 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=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 87 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
2.4 pix Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
2.7 pix fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
2.7 pix fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
Limiting magnitude estimates:
15.3 mag. Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
15.2 mag. Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
12.1 mag. fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
12.3 mag. fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
All-image limiting magnitude estimate: 12.1 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_vSTL
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
############ /tmp/tmp.0YvLAdgjaO (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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/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=47, blended=31903, bad_region=2, passed=206245
Got 206245 stars (including 174023 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 206245 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 4833 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4791 matched stars entering correct_measured_positions(), 4792 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4791 matched stars entering correct_measured_positions(), 206245 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 4832 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4791 matched stars entering correct_measured_positions(), 206245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4791 matched stars entering correct_measured_positions(), 206245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4791 stars left (next iteration limit 5270)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
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=4791 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.422 sigma_q2_arcsec=0.357 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.296 n_q1=1106 n_q2=1277 n_q3=1178 n_q4=1230 worst_quadrant_to_overall_ratio=1.183
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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.fxD2PsAR8A (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_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/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=44, blended=29566, bad_region=0, passed=188594
Got 188594 stars (including 158851 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 188594 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 4841 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4796 matched stars entering correct_measured_positions(), 4797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4796 matched stars entering correct_measured_positions(), 188594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 4840 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4797 matched stars entering correct_measured_positions(), 188594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4797 matched stars entering correct_measured_positions(), 188594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4797 stars left (next iteration limit 5275)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
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=4797 sigma_overall_arcsec=0.514 sigma_q1_arcsec=0.385 sigma_q2_arcsec=0.647 sigma_q3_arcsec=0.512 sigma_q4_arcsec=0.569 n_q1=1146 n_q2=1371 n_q3=1051 n_q4=1229 worst_quadrant_to_overall_ratio=1.258
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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.jvk8afUUEQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
Checking if the catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.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_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
WCS catalog name: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.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=1, blended=351, bad_region=1, passed=15052
Got 15052 stars (including 14672 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat
util/solve_plate_with_UCAC5 got 15052 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4812 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4729 matched stars entering correct_measured_positions(), 4729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4729 matched stars entering correct_measured_positions(), 15052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4814 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4729 matched stars entering correct_measured_positions(), 15052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 4729 matched stars entering correct_measured_positions(), 15052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 4729 stars left (next iteration limit 5201)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4729 robust_rms=14.302 arcsec worst_quadrant_rms=18.905 arcsec
SIP_REFIT: SIP order 3 trial: matched=4729 robust_rms=0.688 arcsec worst_quadrant_rms=0.755 arcsec
SIP_REFIT: SIP order 5 trial: matched=4729 robust_rms=0.558 arcsec worst_quadrant_rms=0.702 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4729 robust_rms_before=0.560 arcsec robust_rms_before_corrected=0.615 arcsec robust_rms_after=0.558 arcsec worst_quadrant_rms_before=0.705 worst_quadrant_rms_after=0.702
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.705 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits N_match=4729 sigma_overall_arcsec=0.598 sigma_q1_arcsec=0.621 sigma_q2_arcsec=0.718 sigma_q3_arcsec=0.562 sigma_q4_arcsec=0.547 n_q1=1146 n_q2=794 n_q3=1397 n_q4=1392 worst_quadrant_to_overall_ratio=1.202
The image catalog is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits -region wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.3U5K1oOBBT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
Checking if the catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
WCS catalog name: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.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=3, blended=402, bad_region=1, passed=16966
Got 16966 stars (including 16534 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat
util/solve_plate_with_UCAC5 got 16966 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 4801 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4726 matched stars entering correct_measured_positions(), 4729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4726 matched stars entering correct_measured_positions(), 16966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 4803 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4726 matched stars entering correct_measured_positions(), 16966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4726 matched stars entering correct_measured_positions(), 16965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 4726 stars left (next iteration limit 5198)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4726 robust_rms=12.541 arcsec worst_quadrant_rms=16.469 arcsec
SIP_REFIT: SIP order 3 trial: matched=4726 robust_rms=0.631 arcsec worst_quadrant_rms=0.692 arcsec
SIP_REFIT: SIP order 5 trial: matched=4726 robust_rms=0.517 arcsec worst_quadrant_rms=0.639 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4726 robust_rms_before=0.519 arcsec robust_rms_before_corrected=0.607 arcsec robust_rms_after=0.517 arcsec worst_quadrant_rms_before=0.640 worst_quadrant_rms_after=0.639
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.640 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits N_match=4726 sigma_overall_arcsec=0.598 sigma_q1_arcsec=0.622 sigma_q2_arcsec=0.760 sigma_q3_arcsec=0.545 sigma_q4_arcsec=0.554 n_q1=1077 n_q2=693 n_q3=1382 n_q4=1574 worst_quadrant_to_overall_ratio=1.269
The image catalog is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits -region wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-34-17_20.00sec_-0.00C_LIGHTs_0093.fits
Saving fully-calibrated image wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Gem-03-Q1b1x1_063602_TTUQ1b1x1_3681101_EL9G0DYm/wcs_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094.fits
Preparing the HTML report for the field Gem-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:07:11.07 +20:59:48.0: 11.33 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:38.13 +26:23:38.1: 12.28 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:13.15 +24:34:30.4: 12.30 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:22.09 +26:47:35.0: 12.22 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:57.72 +26:27:28.2: 12.40 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:30:33.02 +17:37:45.1: 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 06:07:11.07 +20:59:48.0: 11.25 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:57:41.70 +26:50:11.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:45.60 +26:29:33.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.00
Forced photometry filter REJECTED candidate at 06:07:11.07 +20:59:48.0: ref_mag=11.29 +/- 0.00 new_mean_mag=11.3344 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:34.73 +24:31:49.1: 12.88 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:41.16 +26:18:40.2: 13.43 +/- 0.04 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:22.09 +26:47:35.0: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:13.15 +24:34:30.4: 12.27 +/- 0.01 detection
Forced photometry filter KEPT candidate at 06:45:22.09 +26:47:35.0: ref_mag=12.21 +/- 0.01 new_mean_mag=11.1007 delta=1.11 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:57.72 +26:27:28.2: 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 06:43:38.13 +26:23:38.1: 12.20 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:30:33.02 +17:37:45.1: 12.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 06:50:13.15 +24:34:30.4: ref_mag=12.29 +/- 0.01 new_mean_mag=11.3644 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 06:43:57.72 +26:27:28.2: ref_mag=12.38 +/- 0.01 new_mean_mag=11.3465 delta=1.04 (need > 0.90)
Forced photometry filter KEPT candidate at 06:43:38.13 +26:23:38.1: ref_mag=12.24 +/- 0.01 new_mean_mag=11.0958 delta=1.14 (need > 0.90)
Forced photometry filter KEPT candidate at 06:30:33.02 +17:37:45.1: ref_mag=12.13 +/- 0.01 new_mean_mag=11.2051 delta=0.93 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:57:41.70 +26:50:11.4: 12.82 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 05:57:41.70 +26:50:11.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:42:45.60 +26:29:33.8: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 06:42:45.60 +26:29:33.8: ref_mag=12.68 +/- 0.01 new_mean_mag=11.7040 delta=0.98 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:34.73 +24:31:49.1: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter KEPT candidate at 06:50:34.73 +24:31:49.1: ref_mag=12.85 +/- 0.02 new_mean_mag=11.6879 delta=1.16 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:41.16 +26:18:40.2: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:54:33.27 +26:51:12.9: 99.00 +/- 99.00 edge
Forced photometry filter KEPT candidate at 06:43:41.16 +26:18:40.2: ref_mag=13.36 +/- 0.03 new_mean_mag=11.9885 delta=1.37 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:54:33.27 +26:51:12.9: 12.71 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 05:54:33.27 +26:51:12.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:38.84 +26:32:11.7: 13.20 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:18.25 +26:39:57.8: 13.21 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:38.84 +26:32:11.7: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 06:45:38.84 +26:32:11.7: ref_mag=13.19 +/- 0.02 new_mean_mag=11.8688 delta=1.32 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:18.25 +26:39:57.8: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 06:44:18.25 +26:39:57.8: ref_mag=13.23 +/- 0.02 new_mean_mag=11.9691 delta=1.26 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:28.54 +26:43:03.1: 13.14 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:28.54 +26:43:03.1: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 06:44:28.54 +26:43:03.1: ref_mag=13.11 +/- 0.02 new_mean_mag=11.7315 delta=1.38 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:19.25 +24:26:30.7: 13.11 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:19.25 +24:26:30.7: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 06:50:19.25 +24:26:30.7: ref_mag=13.12 +/- 0.02 new_mean_mag=11.6232 delta=1.49 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:20.98 +26:42:03.1: 13.10 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:34.25 +26:01:49.1: 13.05 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:20.98 +26:42:03.1: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 06:44:20.98 +26:42:03.1: ref_mag=13.10 +/- 0.02 new_mean_mag=11.8700 delta=1.23 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:42:34.25 +26:01:49.1: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 06:42:34.25 +26:01:49.1: ref_mag=13.00 +/- 0.02 new_mean_mag=11.8637 delta=1.14 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:03.16 +26:39:24.5: 13.03 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:03.16 +26:39:24.5: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 06:45:03.16 +26:39:24.5: ref_mag=13.01 +/- 0.02 new_mean_mag=11.5850 delta=1.43 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:11.54 +26:27:18.7: 13.02 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:30.33 +26:01:09.7: 12.98 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:11.54 +26:27:18.7: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 06:44:11.54 +26:27:18.7: ref_mag=13.01 +/- 0.02 new_mean_mag=11.7922 delta=1.21 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:30.33 +26:01:09.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 06:43:30.33 +26:01:09.7: ref_mag=12.94 +/- 0.02 new_mean_mag=11.9164 delta=1.02 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:25.21 +26:43:45.6: 12.92 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:34.96 +26:43:05.9: 12.89 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:25.21 +26:43:45.6: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:34.96 +26:43:05.9: 12.80 +/- 0.02 detection
Forced photometry filter KEPT candidate at 06:44:25.21 +26:43:45.6: ref_mag=12.90 +/- 0.02 new_mean_mag=11.8407 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 06:44:34.96 +26:43:05.9: ref_mag=12.84 +/- 0.02 new_mean_mag=11.6399 delta=1.20 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:59.49 +26:33:39.8: 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 06:42:59.49 +26:33:39.8: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry filter KEPT candidate at 06:42:59.49 +26:33:39.8: ref_mag=12.86 +/- 0.02 new_mean_mag=11.8439 delta=1.02 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:43.87 +26:22:04.9: 12.88 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:58.25 +25:50:50.4: 12.86 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:43.87 +26:22:04.9: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter KEPT candidate at 06:43:43.87 +26:22:04.9: ref_mag=12.82 +/- 0.02 new_mean_mag=11.7513 delta=1.07 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:58.25 +25:50:50.4: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 06:43:58.25 +25:50:50.4: ref_mag=12.84 +/- 0.02 new_mean_mag=11.8860 delta=0.95 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:52:57.89 +25:53:56.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:52:57.89 +25:53:56.7: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter KEPT candidate at 06:52:57.89 +25:53:56.7: ref_mag=12.80 +/- 0.02 new_mean_mag=11.8000 delta=1.00 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:43.83 +26:50:07.4: 12.81 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:43.83 +26:50:07.4: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Forced photometry filter KEPT candidate at 06:44:43.83 +26:50:07.4: ref_mag=12.77 +/- 0.02 new_mean_mag=11.6832 delta=1.08 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:54.87 +26:33:17.4: 12.80 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:54.87 +26:33:17.4: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter KEPT candidate at 06:44:54.87 +26:33:17.4: ref_mag=12.80 +/- 0.02 new_mean_mag=11.5587 delta=1.24 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:12.87 +26:20:56.8: 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 06:43:12.87 +26:20:56.8: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Forced photometry filter KEPT candidate at 06:43:12.87 +26:20:56.8: ref_mag=12.78 +/- 0.02 new_mean_mag=11.6246 delta=1.15 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:24.94 +26:47:57.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:46.92 +24:31:05.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:24.94 +26:47:57.2: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Forced photometry filter KEPT candidate at 06:45:24.94 +26:47:57.2: ref_mag=12.77 +/- 0.02 new_mean_mag=11.4652 delta=1.31 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:46.92 +24:31:05.2: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Forced photometry filter KEPT candidate at 06:50:46.92 +24:31:05.2: ref_mag=12.77 +/- 0.02 new_mean_mag=11.6106 delta=1.16 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:46.54 +26:09:14.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:42:46.54 +26:09:14.8: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter KEPT candidate at 06:42:46.54 +26:09:14.8: ref_mag=12.75 +/- 0.02 new_mean_mag=11.7350 delta=1.02 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:44.85 +24:24:02.2: 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 06:50:44.85 +24:24:02.2: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 06:50:44.85 +24:24:02.2: ref_mag=12.63 +/- 0.01 new_mean_mag=11.5651 delta=1.06 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:52:49.23 +25:44:37.8: 12.68 +/- 0.03 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:03.04 +24:57:03.1: 12.68 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:52:49.23 +25:44:37.8: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry filter KEPT candidate at 06:52:49.23 +25:44:37.8: ref_mag=12.68 +/- 0.02 new_mean_mag=11.7270 delta=0.95 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:03.04 +24:57:03.1: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 06:45:03.04 +24:57:03.1: ref_mag=12.65 +/- 0.01 new_mean_mag=11.7000 delta=0.95 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:29.10 +26:16:20.6: 12.66 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:54.55 +26:43:57.4: 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 06:43:29.10 +26:16:20.6: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 06:43:29.10 +26:16:20.6: ref_mag=12.64 +/- 0.01 new_mean_mag=11.4779 delta=1.16 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:54.55 +26:43:57.4: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 06:45:54.55 +26:43:57.4: ref_mag=12.59 +/- 0.01 new_mean_mag=11.5282 delta=1.07 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:42.09 +26:35:21.6: 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 06:45:42.09 +26:35:21.6: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 06:45:42.09 +26:35:21.6: ref_mag=12.60 +/- 0.01 new_mean_mag=11.4522 delta=1.15 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:55:15.56 +23:08:05.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 05:55:15.56 +23:08:05.0: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter KEPT candidate at 05:55:15.56 +23:08:05.0: ref_mag=12.64 +/- 0.02 new_mean_mag=11.7341 delta=0.91 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:48.92 +24:43:26.8: 12.63 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:48.92 +24:43:26.8: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 06:50:48.92 +24:43:26.8: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6176 delta=1.01 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:07.69 +24:33:03.9: 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 06:50:07.69 +24:33:03.9: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter KEPT candidate at 06:50:07.69 +24:33:03.9: ref_mag=12.65 +/- 0.02 new_mean_mag=11.6185 delta=1.03 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:51.09 +25:08:04.9: 12.59 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:51.09 +25:08:04.9: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 06:44:51.09 +25:08:04.9: ref_mag=12.56 +/- 0.01 new_mean_mag=11.5903 delta=0.97 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:01:21.25 +26:34:17.3: 12.61 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:41.53 +24:29:53.3: 12.57 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:01:21.25 +26:34:17.3: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter REJECTED candidate at 06:01:21.25 +26:34:17.3: ref_mag=12.64 +/- 0.02 new_mean_mag=11.7664 delta=0.88 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:41.53 +24:29:53.3: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 06:50:41.53 +24:29:53.3: ref_mag=12.59 +/- 0.01 new_mean_mag=11.4365 delta=1.15 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 05:54:39.64 +22:54:46.3: 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 05:54:39.64 +22:54:46.3: 12.60 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:14.40 +26:26:50.7: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 05:54:39.64 +22:54:46.3: ref_mag=12.56 +/- 0.01 new_mean_mag=11.6092 delta=0.95 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:14.40 +26:26:50.7: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 06:43:14.40 +26:26:50.7: ref_mag=12.45 +/- 0.01 new_mean_mag=11.3722 delta=1.08 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:47:42.89 +24:46:00.1: 12.46 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:24.43 +24:33:13.6: 12.45 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:47:42.89 +24:46:00.1: 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 06:50:24.43 +24:33:13.6: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 06:47:42.89 +24:46:00.1: ref_mag=12.46 +/- 0.01 new_mean_mag=11.4570 delta=1.00 (need > 0.90)
Forced photometry filter KEPT candidate at 06:50:24.43 +24:33:13.6: ref_mag=12.45 +/- 0.01 new_mean_mag=11.4249 delta=1.02 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:59.02 +26:35:24.6: 12.43 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:59.02 +26:35:24.6: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 06:43:59.02 +26:35:24.6: ref_mag=12.39 +/- 0.01 new_mean_mag=11.4338 delta=0.96 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:36.27 +26:21:39.5: 12.40 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:36.27 +26:21:39.5: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 06:43:36.27 +26:21:39.5: ref_mag=12.39 +/- 0.01 new_mean_mag=11.3944 delta=1.00 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:41.48 +26:43:40.8: 12.36 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:13.07 +26:30:12.1: 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 06:44:41.48 +26:43:40.8: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 06:44:41.48 +26:43:40.8: ref_mag=12.36 +/- 0.01 new_mean_mag=11.1781 delta=1.18 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:13.07 +26:30:12.1: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 06:43:13.07 +26:30:12.1: ref_mag=12.33 +/- 0.01 new_mean_mag=11.4030 delta=0.93 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:08.01 +26:47:40.0: 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 06:45:08.01 +26:47:40.0: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter KEPT candidate at 06:45:08.01 +26:47:40.0: ref_mag=12.29 +/- 0.01 new_mean_mag=11.1734 delta=1.11 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:23.03 +26:11:48.4: 12.36 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:23.03 +26:11:48.4: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 06:43:23.03 +26:11:48.4: ref_mag=12.32 +/- 0.01 new_mean_mag=11.3050 delta=1.02 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:52:51.37 +25:48:00.9: 12.35 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:52:51.37 +25:48:00.9: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 06:52:51.37 +25:48:00.9: ref_mag=12.32 +/- 0.01 new_mean_mag=11.4016 delta=0.91 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:07.91 +26:10:19.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:07.91 +26:10:19.2: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 06:44:07.91 +26:10:19.2: ref_mag=12.33 +/- 0.01 new_mean_mag=11.4099 delta=0.92 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:15.26 +24:32:23.2: 12.35 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:15.26 +24:32:23.2: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 06:50:15.26 +24:32:23.2: ref_mag=12.35 +/- 0.01 new_mean_mag=11.3643 delta=0.99 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:52:11.06 +25:59:20.2: 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 06:52:11.06 +25:59:20.2: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 06:52:11.06 +25:59:20.2: ref_mag=12.32 +/- 0.01 new_mean_mag=11.2853 delta=1.04 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:39.24 +26:48:27.6: 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 06:44:39.24 +26:48:27.6: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter KEPT candidate at 06:44:39.24 +26:48:27.6: ref_mag=12.29 +/- 0.01 new_mean_mag=11.2757 delta=1.01 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:51.29 +26:12:31.3: 12.30 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:42:51.29 +26:12:31.3: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 06:42:51.29 +26:12:31.3: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2194 delta=1.04 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:51:47.29 +25:56:04.4: 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 06:51:47.29 +25:56:04.4: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter KEPT candidate at 06:51:47.29 +25:56:04.4: ref_mag=12.28 +/- 0.01 new_mean_mag=11.3120 delta=0.97 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:35.73 +26:43:48.2: 12.28 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:54.80 +26:39:00.7: 12.29 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:35.73 +26:43:48.2: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 06:45:35.73 +26:43:48.2: ref_mag=12.26 +/- 0.01 new_mean_mag=11.0418 delta=1.22 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:54.80 +26:39:00.7: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry filter KEPT candidate at 06:45:54.80 +26:39:00.7: ref_mag=12.27 +/- 0.01 new_mean_mag=11.2071 delta=1.06 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:31:20.75 +17:59:17.3: 12.28 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:31:23.27 +17:58:05.5: 12.23 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:31:20.75 +17:59:17.3: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter KEPT candidate at 06:31:20.75 +17:59:17.3: ref_mag=12.29 +/- 0.01 new_mean_mag=11.2585 delta=1.04 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:31:23.27 +17:58:05.5: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter KEPT candidate at 06:31:23.27 +17:58:05.5: ref_mag=12.25 +/- 0.01 new_mean_mag=11.2809 delta=0.97 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:54.82 +24:48:01.7: 12.23 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:54.82 +24:48:01.7: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter KEPT candidate at 06:44:54.82 +24:48:01.7: ref_mag=12.22 +/- 0.01 new_mean_mag=11.2039 delta=1.01 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:30:53.56 +17:51:47.8: 12.20 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:30:53.56 +17:51:47.8: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry filter KEPT candidate at 06:30:53.56 +17:51:47.8: ref_mag=12.21 +/- 0.01 new_mean_mag=11.2312 delta=0.98 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:40:53.36 +26:14:29.8: 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 06:40:53.36 +26:14:29.8: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter KEPT candidate at 06:40:53.36 +26:14:29.8: ref_mag=12.11 +/- 0.01 new_mean_mag=11.1394 delta=0.97 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:33.54 +24:52:49.3: 12.14 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:26.81 +26:23:07.7: 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 06:44:33.54 +24:52:49.3: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 06:44:33.54 +24:52:49.3: ref_mag=12.13 +/- 0.01 new_mean_mag=11.1968 delta=0.94 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:26.81 +26:23:07.7: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 06:43:26.81 +26:23:07.7: ref_mag=12.00 +/- 0.01 new_mean_mag=11.0216 delta=0.98 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:46:07.18 +26:43:09.0: 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 06:46:07.18 +26:43:09.0: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 06:46:07.18 +26:43:09.0: ref_mag=11.92 +/- 0.01 new_mean_mag=10.9629 delta=0.96 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:50:50.12 +24:32:14.5: 11.88 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:12.16 +26:46:16.2: 11.79 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:50:50.12 +24:32:14.5: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Forced photometry filter KEPT candidate at 06:50:50.12 +24:32:14.5: ref_mag=11.91 +/- 0.01 new_mean_mag=10.9624 delta=0.94 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:12.16 +26:46:16.2: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry filter KEPT candidate at 06:45:12.16 +26:46:16.2: ref_mag=11.78 +/- 0.01 new_mean_mag=10.7398 delta=1.04 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:17.77 +26:43:58.2: 11.64 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:17.77 +26:43:58.2: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.01
Forced photometry filter KEPT candidate at 06:45:17.77 +26:43:58.2: ref_mag=11.61 +/- 0.01 new_mean_mag=10.5864 delta=1.03 (need > 0.90)
Forced photometry on wcs_Gem-03-Q1b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:44:53.71 +26:47:04.9: 11.55 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q1b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:44:53.71 +26:47:04.9: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Forced photometry filter KEPT candidate at 06:44:53.71 +26:47:04.9: ref_mag=11.52 +/- 0.01 new_mean_mag=10.5673 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out131921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out181006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22739.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 79s
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: 38s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 230759_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 230759_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 06:40:05.50 +26:15:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 230760_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 230760_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 230765_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 230765_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 06:59:22.65 +25:14:08.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 231083_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 231083_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 05:54:52.93 +19:44:20.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16268_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 16268_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160010_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 160010_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167966_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 167966_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153030_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 153030_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166426_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 166426_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166210_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 166210_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152059_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 152059_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169126_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 169126_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219408_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 219408_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219087_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 219087_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219074_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 219074_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219045_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 219045_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 05:56:59.13 +26:51:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218864_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 218864_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 05:56:55.24 +26:51:46.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218776_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 218776_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 05:54:37.01 +26:49:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164885_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 164885_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163042_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 163042_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162250_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 162250_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150251_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 150251_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161884_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 161884_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174635_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 174635_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162698_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 162698_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167240_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 167240_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175593_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 175593_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110234_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 110234_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 05:56:11.21 +21:51:43.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161384_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 161384_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162208_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 162208_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164711_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 164711_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168149_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 168149_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178835_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 178835_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177254_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 177254_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159540_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 159540_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164595_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 164595_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170288_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 170288_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147564_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 147564_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 05:54:40.36 +23:43:08.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159986_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 159986_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151856_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 151856_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173249_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 173249_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149524_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 149524_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181006_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 181006_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195959_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 195959_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170111_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 170111_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162206_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 162206_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164103_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 164103_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136031_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 136031_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155952_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 155952_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152577_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 152577_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192321_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 192321_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156747_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 156747_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151516_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 151516_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131921_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 131921_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166533_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 166533_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20425_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 20425_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 06:32:33.69 +17:50:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200496_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 200496_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152646_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 152646_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164363_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 164363_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168288_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 168288_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161356_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 161356_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165517_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 165517_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160332_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 160332_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171527_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 171527_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179901_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 179901_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172108_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 172108_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152294_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 152294_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175816_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 175816_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159919_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 159919_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171162_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 171162_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176505_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 176505_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163003_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 163003_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161510_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 161510_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22739_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 22739_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22262_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 22262_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198796_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 198796_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20510_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 20510_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45053_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 45053_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 05:57:02.98 +18:42:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171190_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 171190_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197338_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 197338_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168279_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 168279_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161190_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 161190_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152551_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 152551_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160875_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 160875_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161406_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 161406_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160854_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
Preparing report for the candidate 160854_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121149_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094
The candidate 121149_fd_Gem-03-Q1b1x1_2026-09-10_06-35-15_20.00sec_-0.00C_LIGHTs_0094 did not pass the final checks
**** FOUND 06:41:57.02 +22:56:10.5 in the exclusion list exclusion_list_local.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 122s
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 ####
06:41:56.99 +22:56:10.9
05:54:39.64 +22:54:46.3
05:55:15.56 +23:08:05.0
06:50:44.85 +24:24:02.2
06:50:19.25 +24:26:30.7
06:50:41.53 +24:29:53.3
06:50:46.92 +24:31:05.2
06:50:34.73 +24:31:49.1
06:50:15.26 +24:32:23.2
06:50:50.12 +24:32:14.5
06:50:07.69 +24:33:03.9
06:50:24.43 +24:33:13.6
06:50:13.15 +24:34:30.4
06:50:48.92 +24:43:26.8
06:44:43.83 +26:50:07.4
06:44:39.24 +26:48:27.6
06:45:24.94 +26:47:57.2
06:45:22.09 +26:47:35.0
06:45:08.01 +26:47:40.0
06:44:53.71 +26:47:04.9
06:45:12.16 +26:46:16.2
06:46:07.18 +26:43:09.0
06:44:41.48 +26:43:40.8
06:44:25.21 +26:43:45.6
06:45:17.77 +26:43:58.2
06:45:35.73 +26:43:48.2
06:44:20.98 +26:42:03.1
06:45:54.55 +26:43:57.4
06:44:34.96 +26:43:05.9
06:44:28.54 +26:43:03.1
06:30:33.02 +17:37:45.1
06:45:03.16 +26:39:24.5
06:45:54.80 +26:39:00.7
06:44:18.25 +26:39:57.8
06:45:42.09 +26:35:21.6
06:43:59.02 +26:35:24.6
06:44:54.87 +26:33:17.4
06:42:59.49 +26:33:39.8
06:45:38.84 +26:32:11.7
06:43:13.07 +26:30:12.1
06:42:45.60 +26:29:33.8
06:43:57.72 +26:27:28.2
06:43:14.40 +26:26:50.7
06:44:11.54 +26:27:18.7
06:43:38.13 +26:23:38.1
06:43:43.87 +26:22:04.9
06:43:26.81 +26:23:07.7
06:43:36.27 +26:21:39.5
06:43:41.16 +26:18:40.2
06:43:29.10 +26:16:20.6
06:43:12.87 +26:20:56.8
06:42:51.29 +26:12:31.3
06:40:53.36 +26:14:29.8
06:43:23.03 +26:11:48.4
06:44:07.91 +26:10:19.2
06:42:46.54 +26:09:14.8
06:42:34.25 +26:01:49.1
06:43:30.33 +26:01:09.7
06:52:11.06 +25:59:20.2
06:51:47.29 +25:56:04.4
06:52:57.89 +25:53:56.7
06:43:58.25 +25:50:50.4
06:52:51.37 +25:48:00.9
06:52:49.23 +25:44:37.8
06:44:51.09 +25:08:04.9
06:45:03.04 +24:57:03.1
06:44:33.54 +24:52:49.3
06:44:54.82 +24:48:01.7
06:47:42.89 +24:46:00.1
06:30:53.56 +17:51:47.8
06:31:23.27 +17:58:05.5
06:31:20.75 +17:59:17.3
########### 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 ####
06:41:56.99 +22:56:10.9
06:30:33.02 +17:37:45.1
06:45:22.09 +26:47:35.0
06:43:38.13 +26:23:38.1
06:50:13.15 +24:34:30.4
06:43:57.72 +26:27:28.2
06:42:45.60 +26:29:33.8
06:50:34.73 +24:31:49.1
06:43:41.16 +26:18:40.2
06:45:38.84 +26:32:11.7
06:44:18.25 +26:39:57.8
06:44:28.54 +26:43:03.1
06:50:19.25 +24:26:30.7
06:44:20.98 +26:42:03.1
06:42:34.25 +26:01:49.1
06:45:03.16 +26:39:24.5
06:44:11.54 +26:27:18.7
06:43:30.33 +26:01:09.7
06:44:25.21 +26:43:45.6
06:44:34.96 +26:43:05.9
06:42:59.49 +26:33:39.8
06:43:43.87 +26:22:04.9
06:43:58.25 +25:50:50.4
06:52:57.89 +25:53:56.7
06:44:43.83 +26:50:07.4
06:44:54.87 +26:33:17.4
06:43:12.87 +26:20:56.8
06:45:24.94 +26:47:57.2
06:50:46.92 +24:31:05.2
06:42:46.54 +26:09:14.8
06:50:44.85 +24:24:02.2
06:52:49.23 +25:44:37.8
06:45:03.04 +24:57:03.1
06:43:29.10 +26:16:20.6
06:45:54.55 +26:43:57.4
06:45:42.09 +26:35:21.6
05:55:15.56 +23:08:05.0
06:50:48.92 +24:43:26.8
06:50:07.69 +24:33:03.9
06:44:51.09 +25:08:04.9
06:50:41.53 +24:29:53.3
05:54:39.64 +22:54:46.3
06:43:14.40 +26:26:50.7
06:47:42.89 +24:46:00.1
06:50:24.43 +24:33:13.6
06:43:59.02 +26:35:24.6
06:43:36.27 +26:21:39.5
06:44:41.48 +26:43:40.8
06:43:13.07 +26:30:12.1
06:45:08.01 +26:47:40.0
06:43:23.03 +26:11:48.4
06:52:51.37 +25:48:00.9
06:44:07.91 +26:10:19.2
06:50:15.26 +24:32:23.2
06:52:11.06 +25:59:20.2
06:44:39.24 +26:48:27.6
06:42:51.29 +26:12:31.3
06:51:47.29 +25:56:04.4
06:45:54.80 +26:39:00.7
06:45:35.73 +26:43:48.2
06:31:20.75 +17:59:17.3
06:31:23.27 +17:58:05.5
06:44:54.82 +24:48:01.7
06:30:53.56 +17:51:47.8
06:40:53.36 +26:14:29.8
06:44:33.54 +24:52:49.3
06:43:26.81 +26:23:07.7
06:46:07.18 +26:43:09.0
06:50:50.12 +24:32:14.5
06:45:12.16 +26:46:16.2
06:45:17.77 +26:43:58.2
06:44:53.71 +26:47:04.9
###################################################################################
06:41:56.99 +22:56:10.9 -- asteroid (will NOT add it to exclusion list)
06:30:33.02 +17:37:45.1 -- not an asteroid (will add it to exclusion list)
06:45:22.09 +26:47:35.0 -- not an asteroid (will add it to exclusion list)
06:43:38.13 +26:23:38.1 -- not an asteroid (will add it to exclusion list)
06:50:13.15 +24:34:30.4 -- not an asteroid (will add it to exclusion list)
06:43:57.72 +26:27:28.2 -- not an asteroid (will add it to exclusion list)
06:42:45.60 +26:29:33.8 -- not an asteroid (will add it to exclusion list)
06:50:34.73 +24:31:49.1 -- not an asteroid (will add it to exclusion list)
06:43:41.16 +26:18:40.2 -- not an asteroid (will add it to exclusion list)
06:45:38.84 +26:32:11.7 -- not an asteroid (will add it to exclusion list)
06:44:18.25 +26:39:57.8 -- not an asteroid (will add it to exclusion list)
06:44:28.54 +26:43:03.1 -- not an asteroid (will add it to exclusion list)
06:50:19.25 +24:26:30.7 -- not an asteroid (will add it to exclusion list)
06:44:20.98 +26:42:03.1 -- not an asteroid (will add it to exclusion list)
06:42:34.25 +26:01:49.1 -- not an asteroid (will add it to exclusion list)
06:45:03.16 +26:39:24.5 -- not an asteroid (will add it to exclusion list)
06:44:11.54 +26:27:18.7 -- not an asteroid (will add it to exclusion list)
06:43:30.33 +26:01:09.7 -- not an asteroid (will add it to exclusion list)
06:44:25.21 +26:43:45.6 -- not an asteroid (will add it to exclusion list)
06:44:34.96 +26:43:05.9 -- not an asteroid (will add it to exclusion list)
06:42:59.49 +26:33:39.8 -- not an asteroid (will add it to exclusion list)
06:43:43.87 +26:22:04.9 -- not an asteroid (will add it to exclusion list)
06:43:58.25 +25:50:50.4 -- not an asteroid (will add it to exclusion list)
06:52:57.89 +25:53:56.7 -- not an asteroid (will add it to exclusion list)
06:44:43.83 +26:50:07.4 -- not an asteroid (will add it to exclusion list)
06:44:54.87 +26:33:17.4 -- not an asteroid (will add it to exclusion list)
06:43:12.87 +26:20:56.8 -- not an asteroid (will add it to exclusion list)
06:45:24.94 +26:47:57.2 -- not an asteroid (will add it to exclusion list)
06:50:46.92 +24:31:05.2 -- not an asteroid (will add it to exclusion list)
06:42:46.54 +26:09:14.8 -- not an asteroid (will add it to exclusion list)
06:50:44.85 +24:24:02.2 -- not an asteroid (will add it to exclusion list)
06:52:49.23 +25:44:37.8 -- not an asteroid (will add it to exclusion list)
06:45:03.04 +24:57:03.1 -- not an asteroid (will add it to exclusion list)
06:43:29.10 +26:16:20.6 -- not an asteroid (will add it to exclusion list)
06:45:54.55 +26:43:57.4 -- not an asteroid (will add it to exclusion list)
06:45:42.09 +26:35:21.6 -- not an asteroid (will add it to exclusion list)
05:55:15.56 +23:08:05.0 -- not an asteroid (will add it to exclusion list)
06:50:48.92 +24:43:26.8 -- not an asteroid (will add it to exclusion list)
06:50:07.69 +24:33:03.9 -- not an asteroid (will add it to exclusion list)
06:44:51.09 +25:08:04.9 -- not an asteroid (will add it to exclusion list)
06:50:41.53 +24:29:53.3 -- not an asteroid (will add it to exclusion list)
05:54:39.64 +22:54:46.3 -- not an asteroid (will add it to exclusion list)
06:43:14.40 +26:26:50.7 -- not an asteroid (will add it to exclusion list)
06:47:42.89 +24:46:00.1 -- not an asteroid (will add it to exclusion list)
06:50:24.43 +24:33:13.6 -- not an asteroid (will add it to exclusion list)
06:43:59.02 +26:35:24.6 -- not an asteroid (will add it to exclusion list)
06:43:36.27 +26:21:39.5 -- not an asteroid (will add it to exclusion list)
06:44:41.48 +26:43:40.8 -- not an asteroid (will add it to exclusion list)
06:43:13.07 +26:30:12.1 -- not an asteroid (will add it to exclusion list)
06:45:08.01 +26:47:40.0 -- not an asteroid (will add it to exclusion list)
06:43:23.03 +26:11:48.4 -- not an asteroid (will add it to exclusion list)
06:52:51.37 +25:48:00.9 -- not an asteroid (will add it to exclusion list)
06:44:07.91 +26:10:19.2 -- not an asteroid (will add it to exclusion list)
06:50:15.26 +24:32:23.2 -- not an asteroid (will add it to exclusion list)
06:52:11.06 +25:59:20.2 -- not an asteroid (will add it to exclusion list)
06:44:39.24 +26:48:27.6 -- not an asteroid (will add it to exclusion list)
06:42:51.29 +26:12:31.3 -- not an asteroid (will add it to exclusion list)
06:51:47.29 +25:56:04.4 -- not an asteroid (will add it to exclusion list)
06:45:54.80 +26:39:00.7 -- not an asteroid (will add it to exclusion list)
06:45:35.73 +26:43:48.2 -- not an asteroid (will add it to exclusion list)
06:31:20.75 +17:59:17.3 -- asteroid (will NOT add it to exclusion list)
06:31:23.27 +17:58:05.5 -- asteroid (will NOT add it to exclusion list)
06:44:54.82 +24:48:01.7 -- not an asteroid (will add it to exclusion list)
06:30:53.56 +17:51:47.8 -- not an asteroid (will add it to exclusion list)
06:40:53.36 +26:14:29.8 -- not an asteroid (will add it to exclusion list)
06:44:33.54 +24:52:49.3 -- not an asteroid (will add it to exclusion list)
06:43:26.81 +26:23:07.7 -- not an asteroid (will add it to exclusion list)
06:46:07.18 +26:43:09.0 -- not an asteroid (will add it to exclusion list)
06:50:50.12 +24:32:14.5 -- not an asteroid (will add it to exclusion list)
06:45:12.16 +26:46:16.2 -- not an asteroid (will add it to exclusion list)
06:45:17.77 +26:43:58.2 -- not an asteroid (will add it to exclusion list)
06:44:53.71 +26:47:04.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:54:39.64 +22:54:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:15.56 +23:08:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:33.02 +17:37:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:53.56 +17:51:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:53.36 +26:14:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:34.25 +26:01:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:45.60 +26:29:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:46.54 +26:09:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:51.29 +26:12:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:59.49 +26:33:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:12.87 +26:20:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:13.07 +26:30:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:14.40 +26:26:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:23.03 +26:11:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:26.81 +26:23:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:29.10 +26:16:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:30.33 +26:01:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:36.27 +26:21:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:38.13 +26:23:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:41.16 +26:18:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:43.87 +26:22:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:57.72 +26:27:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:58.25 +25:50:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:59.02 +26:35:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:07.91 +26:10:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:11.54 +26:27:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:18.25 +26:39:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:20.98 +26:42:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:25.21 +26:43:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:28.54 +26:43:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:33.54 +24:52:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:34.96 +26:43:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:39.24 +26:48:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:41.48 +26:43:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:43.83 +26:50:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:51.09 +25:08:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:53.71 +26:47:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:54.82 +24:48:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:54.87 +26:33:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:03.04 +24:57:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:03.16 +26:39:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:08.01 +26:47:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.16 +26:46:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:17.77 +26:43:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:22.09 +26:47:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:24.94 +26:47:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:35.73 +26:43:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:38.84 +26:32:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:42.09 +26:35:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:54.55 +26:43:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:54.80 +26:39:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:07.18 +26:43:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:42.89 +24:46:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:07.69 +24:33:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:13.15 +24:34:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:15.26 +24:32:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:19.25 +24:26:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:24.43 +24:33:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:34.73 +24:31:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.53 +24:29:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:44.85 +24:24:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:46.92 +24:31:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:48.92 +24:43:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:50.12 +24:32:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:47.29 +25:56:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:11.06 +25:59:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:49.23 +25:44:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:51.37 +25:48:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:57.89 +25:53:56.7 -- 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)
05:54:39.64 +22:54:46.3 -- not a known variable star
05:55:15.56 +23:08:05.0 -- not a known variable star
06:30:33.02 +17:37:45.1 -- not a known variable star
06:30:53.56 +17:51:47.8 -- not a known variable star
06:40:53.36 +26:14:29.8 -- a known variable star
06:42:34.25 +26:01:49.1 -- not a known variable star
06:42:45.60 +26:29:33.8 -- not a known variable star
06:42:46.54 +26:09:14.8 -- not a known variable star
06:42:51.29 +26:12:31.3 -- not a known variable star
06:42:59.49 +26:33:39.8 -- not a known variable star
06:43:12.87 +26:20:56.8 -- not a known variable star
06:43:13.07 +26:30:12.1 -- not a known variable star
06:43:14.40 +26:26:50.7 -- a known variable star
06:43:23.03 +26:11:48.4 -- not a known variable star
06:43:26.81 +26:23:07.7 -- not a known variable star
06:43:29.10 +26:16:20.6 -- not a known variable star
06:43:30.33 +26:01:09.7 -- not a known variable star
06:43:36.27 +26:21:39.5 -- not a known variable star
06:43:38.13 +26:23:38.1 -- not a known variable star
06:43:41.16 +26:18:40.2 -- not a known variable star
06:43:43.87 +26:22:04.9 -- not a known variable star
06:43:57.72 +26:27:28.2 -- not a known variable star
06:43:58.25 +25:50:50.4 -- not a known variable star
06:43:59.02 +26:35:24.6 -- not a known variable star
06:44:07.91 +26:10:19.2 -- not a known variable star
06:44:11.54 +26:27:18.7 -- not a known variable star
06:44:18.25 +26:39:57.8 -- a known variable star
06:44:20.98 +26:42:03.1 -- not a known variable star
06:44:25.21 +26:43:45.6 -- not a known variable star
06:44:28.54 +26:43:03.1 -- not a known variable star
06:44:33.54 +24:52:49.3 -- not a known variable star
06:44:34.96 +26:43:05.9 -- a known variable star
06:44:39.24 +26:48:27.6 -- not a known variable star
06:44:41.48 +26:43:40.8 -- not a known variable star
06:44:43.83 +26:50:07.4 -- not a known variable star
06:44:51.09 +25:08:04.9 -- not a known variable star
06:44:53.71 +26:47:04.9 -- not a known variable star
06:44:54.82 +24:48:01.7 -- not a known variable star
06:44:54.87 +26:33:17.4 -- not a known variable star
06:45:03.04 +24:57:03.1 -- not a known variable star
06:45:03.16 +26:39:24.5 -- not a known variable star
06:45:08.01 +26:47:40.0 -- not a known variable star
06:45:12.16 +26:46:16.2 -- not a known variable star
06:45:17.77 +26:43:58.2 -- a known variable star
06:45:22.09 +26:47:35.0 -- a known variable star
06:45:24.94 +26:47:57.2 -- a known variable star
06:45:35.73 +26:43:48.2 -- not a known variable star
06:45:38.84 +26:32:11.7 -- not a known variable star
06:45:42.09 +26:35:21.6 -- not a known variable star
06:45:54.55 +26:43:57.4 -- not a known variable star
06:45:54.80 +26:39:00.7 -- not a known variable star
06:46:07.18 +26:43:09.0 -- not a known variable star
06:47:42.89 +24:46:00.1 -- not a known variable star
06:50:07.69 +24:33:03.9 -- not a known variable star
06:50:13.15 +24:34:30.4 -- not a known variable star
06:50:15.26 +24:32:23.2 -- not a known variable star
06:50:19.25 +24:26:30.7 -- not a known variable star
06:50:24.43 +24:33:13.6 -- a known variable star
06:50:34.73 +24:31:49.1 -- not a known variable star
06:50:41.53 +24:29:53.3 -- not a known variable star
06:50:44.85 +24:24:02.2 -- not a known variable star
06:50:46.92 +24:31:05.2 -- not a known variable star
06:50:48.92 +24:43:26.8 -- not a known variable star
06:50:50.12 +24:32:14.5 -- not a known variable star
06:51:47.29 +25:56:04.4 -- not a known variable star
06:52:11.06 +25:59:20.2 -- not a known variable star
06:52:49.23 +25:44:37.8 -- not a known variable star
06:52:51.37 +25:48:00.9 -- a known variable star
06:52:57.89 +25:53:56.7 -- not a known variable star
Found 60 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
69 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 69 (excluding asteroids and hot pixels, 60 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)2461293.98226567 -observatory V36
11:58:35.85 +00:58:39.0 Mercury (-0.7mag)
13:43:49.50 -15:41:26.6 Venus (-4.7mag)
07:22:33.02 +22:46:00.7 Mars (1.2mag)
09:11:39.42 +16:46:29.1 Jupiter (-1.8mag)
00:50:58.77 +02:33:19.6 Saturn (0.4mag)
04:13:42.59 +21:02:03.2 Uranus (5.7mag)
00:13:26.52 -00:05:16.7 Neptune (7.7mag)
20:25:22.81 -23:40:19.0 Pluto (14.5mag)
10:44:02.36 +06:52:43.7 Moon (99.9mag)
-rw-r--r-- 1 apache apache 362 Sep 10 06:38 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461293.98226567:
09:11:46.81 +16:45:52.9 Io (6.2mag)
09:11:41.38 +16:46:20.5 Europa (6.3mag)
09:11:28.23 +16:47:27.3 Ganymede (5.7mag)
09:11:40.50 +16:46:25.8 Callisto (6.9mag)
09:09:32.49 +17:04:22.3 Himalia (15.7mag)
09:11:39.76 +16:46:27.8 Thebe (16.6mag)
09:09:07.57 +16:58:15.6 Elara (17.7mag)
09:15:28.26 +16:13:08.4 Pasiphae (17.9mag)
09:12:30.60 +17:05:08.4 Carme (19.0mag)
00:50:44.66 +02:33:23.9 Titan (8.3mag)
00:50:57.35 +02:33:24.3 Rhea (9.6mag)
00:51:05.14 +02:35:30.4 Iapetus (11.0mag)
00:51:13.41 +02:33:14.1 Hyperion (14.3mag)
00:49:42.26 +02:22:46.4 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 10 06:38 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461293.98226567:
22:29:25.38 +04:15:02.9 JWST
18:37:33.61 +16:37:08.9 Chandra
07:05:12.85 -05:45:48.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 10 06:38 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461293.98226567 -observatory V36
03:42:12.40 +19:28:56.9 17.3mag P/1996 R2 (Lagerkvist)
18:04:07.12 -34:09:05.0 14.4mag P/2010 H2 (Vales)
07:21:50.76 -70:28:47.7 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:01.76 +33:47:00.9 17.7mag C/2017 K2 (PANSTARRS)
22:10:58.27 +28:16:32.5 17.5mag C/2022 E2 (ATLAS)
07:12:33.87 +25:55:13.5 16.9mag C/2022 N2 (PANSTARRS)
10:52:25.84 +27:06:49.4 17.1mag C/2022 QE78 (ATLAS)
09:50:41.06 +05:12:55.3 18.0mag C/2022 R6 (PANSTARRS)
15:28:44.90 -15:55:42.3 14.9mag C/2023 R1 (PANSTARRS)
08:41:08.58 +33:05:34.2 15.8mag C/2024 E1 (Wierzchos)
15:07:01.94 +15:17:11.4 17.9mag C/2024 G6 (ATLAS)
18:31:43.15 +43:02:50.1 13.7mag C/2024 J3 (ATLAS)
20:21:52.70 +49:07:06.9 17.4mag C/2024 R4 (PANSTARRS)
05:37:15.16 -13:04:18.7 15.1mag C/2024 T5 (ATLAS)
07:12:40.33 +17:54:06.9 17.8mag C/2025 J1 (Borisov)
11:23:08.54 +18:31:10.1 16.8mag C/2025 V2 (Rankin)
13:22:16.50 -00:08:30.4 16.8mag C/2025 Y1 (ATLAS)
16:50:01.83 +73:29:40.7 16.0mag C/2026 A2 (Bok)
03:04:06.34 +46:01:29.3 17.5mag C/2026 B2 (Sun-Gao)
12:16:14.01 +11:32:36.7 17.5mag A/2026 E1
22:28:38.57 -35:11:58.5 13.5mag 10P/Tempel
01:24:27.25 +37:39:34.5 17.8mag 11P/Tempel-Swift-LINEAR
11:50:18.58 -05:42:31.4 16.3mag 29P/Schwassmann-Wachmann
12:14:59.23 -06:05:58.8 17.7mag 63P/Wild
06:45:26.10 +19:00:12.4 13.7mag 78P/Gehrels
03:17:18.42 +15:01:47.8 17.2mag 88P/Howell
05:48:52.68 +29:50:33.7 16.9mag 112P/Urata-Niijima
07:41:11.30 +23:59:05.4 15.9mag 114P/Wiseman-Skiff
10:34:59.29 +20:11:18.7 14.8mag 123P/West-Hartley
12:53:38.94 -22:26:32.6 17.5mag 124P/Mrkos
06:21:13.49 +20:32:17.6 15.9mag 128P/Shoemaker-Holt
02:18:43.98 -17:10:34.9 14.9mag 161P/Hartley-IRAS
09:01:48.98 +37:28:12.5 16.4mag 162P/Siding Spring
09:33:18.91 +11:51:42.1 13.2mag 169P/NEAT
03:26:56.10 +08:12:07.2 14.5mag 220P/McNaught
04:56:34.96 +37:18:16.3 15.2mag 260P/McNaught
08:40:21.80 +35:21:22.1 17.3mag 295P/LINEAR
15:27:20.38 -00:36:21.8 17.9mag 391P/Kowalski
09:30:31.48 +16:41:16.4 17.8mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.0K Sep 10 06:38 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
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
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
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
-rw-r--r-- 1 apache apache 5.7K Sep 10 06:38 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 10 06:38 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
01:10:34.560 -00:57:04.24 AT 2026yyl 2026-08-06.84 21.95
23:32:11.290 +02:22:43.17 AT 2026yyk 2026-08-06.82 22.15
00:08:51.810 +05:23:51.48 AT 2026yyj 2026-08-06.76 22.29
22:56:29.190 +05:38:34.33 AT 2026yyi 2026-08-06.74 22.59
00:15:40.360 +03:16:53.74 AT 2026yyh 2026-08-04.79 21.17
23:43:25.860 +04:21:29.59 AT 2026yyg 2026-08-04.79 20.76
01:06:50.820 +00:11:19.23 AT 2026yyf 2026-08-01.81 21.09
13:53:44.240 -01:14:56.96 AT 2026yye 2026-07-21.61 20.99
23:54:21.350 +02:49:56.21 AT 2026yyd 2026-07-15.87 22.7
23:59:00.130 +05:02:18.24 AT 2026yyc 2026-08-09.84 21.93
02:17:16.710 -00:36:33.05 AT 2026yyb 2026-07-30.82 20.03
02:27:18.740 +05:57:45.58 AT 2026yya 2026-08-01.84 20.95
01:29:14.660 +04:56:12.14 AT 2026yxz 2026-08-06.84 21.5
05:02:13.153 +13:11:04.42 AT 2026yxy 2026-07-19.50 18.8535
22:01:35.905 -00:50:35.09 AT 2026yxx 2026-08-12.32 19.906
16:14:10.014 -14:08:40.56 AT 2026yxw 2026-08-12.88 19.268
02:19:09.961 +30:43:26.21 AT 2026yxv 2026-08-14.56 19.34
13:13:44.418 +06:59:28.07 AT 2026yxu 2026-08-05.16 19.7272
14:52:44.979 +53:35:27.83 AT 2026yxt 2026-08-05.18 20.8609
00:56:58.931 +27:08:48.44 SN 2026yxs 2026-08-15.06 19.27
-rw-r--r-- 1 apache apache 88K Sep 10 06:38 tns_transients_list.txt
