This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM
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 08 06.3057 2461258.8057 11.72 06:59:43.71 +68:29:44.9
146.95259 25.85163 galactic Cam Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:59:43.71 +68:29:44.9 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.028 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:59:43.71 +68:29:44.9: 12.64 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:59:43.71 +68:29:44.9: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.66 06:49:38.45 +67:46:49.0
147.55022 24.80199 galactic Cam Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1102814114029512960 | 06:49:38.36 +67:46:48.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.668+/-0.034 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:49:38.45 +67:46:49.0: 12.67 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:49:38.45 +67:46:49.0: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1102814114029512960,2461258.8057,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1102814114029512960 20260806.3057 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.75 06:35:30.37 +66:49:57.7
148.22101 23.25930 galactic Cam Second-epoch detections are separated by 1.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:35:30.37 +66:49:57.7 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.029 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:35:30.37 +66:49:57.7: 12.76 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:35:30.37 +66:49:57.7: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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,2461258.8057,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.71 07:13:53.42 +69:06:52.7
146.44088 27.19736 galactic Cam Second-epoch detections are separated by 0.4" and 5.7 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 | 07:13:53.42 +69:06:52.7 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.026 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:13:53.42 +69:06:52.7: 12.78 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:13:53.42 +69:06:52.7: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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,2461258.8057,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.79 07:36:53.59 +69:19:06.4
146.31191 29.24416 galactic Cam Second-epoch detections are separated by 0.8" and 5.9 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 | 07:36:53.59 +69:19:06.4 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:36:53.59 +69:19:06.4: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:36:53.59 +69:19:06.4: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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,2461258.8057,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.84 07:22:13.49 +69:43:12.2
145.81908 27.97146 galactic Cam Second-epoch detections are separated by 2.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:22:13.49 +69:43:12.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:22:13.49 +69:43:12.2: 12.87 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:22:13.49 +69:43:12.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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,2461258.8057,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.86 07:12:16.39 +69:02:11.2
146.51294 27.04621 galactic Cam Second-epoch detections are separated by 1.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:12:16.39 +69:02:11.2 (user input) | T | P | (position from user input) J-Ks=0.661+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:16.39 +69:02:11.2: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:16.39 +69:02:11.2: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 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
target,2461258.8057,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.95 07:16:59.37 +68:23:57.3
147.27073 27.41379 galactic Cam Second-epoch detections are separated by 1.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:16:59.37 +68:23:57.3 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.032 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:16:59.37 +68:23:57.3: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:16:59.37 +68:23:57.3: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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,2461258.8057,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.90 07:27:10.47 +69:12:45.4
146.41615 28.38236 galactic Cam Second-epoch detections are separated by 1.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:27:10.47 +69:12:45.4 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:27:10.47 +69:12:45.4: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:27:10.47 +69:12:45.4: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 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
target,2461258.8057,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.09 07:42:38.33 +69:52:50.6
145.65573 29.73464 galactic Cam Second-epoch detections are separated by 1.2" and 5.9 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 | 07:42:38.33 +69:52:50.6 (user input) | T | P | (position from user input) J-Ks=0.629+/-0.031 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:42:38.33 +69:52:50.6: 13.24 +/- 0.03 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:42:38.33 +69:52:50.6: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.12 07:08:40.22 +68:28:15.2
147.10359 26.66061 galactic Cam Second-epoch detections are separated by 1.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:08:40.22 +68:28:15.2 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:08:40.22 +68:28:15.2: 13.38 +/- 0.03 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:08:40.22 +68:28:15.2: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.07 06:56:17.55 +67:04:48.4
148.44119 25.29793 galactic Cam Second-epoch detections are separated by 2.5" and 5.5 pix
The object was found in VSX 1" V0465 Cam
Type: EA
# Max. Min./Amp. JD0 Period
13.400 R1 14.500 R1 2451567.82000 1.936530000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:56:17.55 +67:04:48.4: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:56:17.55 +67:04:48.4: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0465 Cam,2461258.8057,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0465 Cam 20260806.3057 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.12 07:10:50.86 +68:48:23.3
146.75491 26.89518 galactic Cam Second-epoch detections are separated by 3.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:10:50.86 +68:48:23.3 (user input) | T | P | (position from user input) J-Ks=0.469+/-0.027 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:10:50.86 +68:48:23.3: 13.44 +/- 0.03 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:10:50.86 +68:48:23.3: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 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,2461258.8057,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.12 07:31:17.48 +69:44:00.9
145.83395 28.75680 galactic Cam Second-epoch detections are separated by 2.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:31:17.48 +69:44:00.9 (user input) | T | P | (position from user input) J-Ks=0.535+/-0.029 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:31:17.48 +69:44:00.9: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:31:17.48 +69:44:00.9: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.94 07:18:16.63 +69:27:16.0
146.09480 27.61155 galactic Cam Second-epoch detections are separated by 2.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:18:16.63 +69:27:16.0 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.029 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:16.63 +69:27:16.0: 13.26 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:16.63 +69:27:16.0: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 12.05 07:25:24.69 +69:55:46.4
145.59579 28.25535 galactic Cam Second-epoch detections are separated by 1.0" and 5.8 pix
The object was found in VSX 0" Gaia DR3 1108943448974794624
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.020 G 13.050 G F
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:25:24.69 +69:55:46.4: 13.24 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:25:24.69 +69:55:46.4: 13.22 +/- 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
Gaia DR3 1108943448974794624,2461258.8057,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108943448974794624 20260806.3057 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.05 07:27:43.80 +70:22:54.8
145.08886 28.46588 galactic Cam Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:27:43.80 +70:22:54.8 (user input) | T | P | (position from user input) J-Ks=0.382+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:27:43.80 +70:22:54.8: 13.22 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:27:43.80 +70:22:54.8: 13.25 +/- 0.02 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
target,2461258.8057,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.01 07:19:03.99 +68:28:18.0
147.20676 27.60987 galactic Cam Second-epoch detections are separated by 1.0" and 5.9 pix
The object was found in VSX 2" Gaia DR3 1108381426735302016
Type: ROT
# Max. Min./Amp. JD0 Period
13.320 G 13.380 G K
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:19:03.99 +68:28:18.0: 13.22 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:19:03.99 +68:28:18.0: 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
Gaia DR3 1108381426735302016,2461258.8057,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108381426735302016 20260806.3057 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 08 06.3057 2461258.8057 12.01 07:26:36.83 +69:55:51.2
145.59838 28.35848 galactic Cam Second-epoch detections are separated by 1.6" and 5.9 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 | 07:26:36.83 +69:55:51.2 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:36.83 +69:55:51.2: 13.18 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:36.83 +69:55:51.2: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 12.04 07:12:31.55 +68:43:37.1
146.86122 27.03812 galactic Cam Second-epoch detections are separated by 1.9" and 5.4 pix
The object was found in VSX 1" Gaia DR3 1109062299311163776
Type: ROT
# Max. Min./Amp. JD0 Period
12.810 G 12.850 G 3.413640000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:31.55 +68:43:37.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:31.55 +68:43:37.1: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1109062299311163776,2461258.8057,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109062299311163776 20260806.3057 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.97 07:20:20.58 +69:39:57.1
145.86988 27.80539 galactic Cam Second-epoch detections are separated by 0.1" and 5.7 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 | 07:20:20.58 +69:39:57.1 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:20.58 +69:39:57.1: 13.13 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:20.58 +69:39:57.1: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.90 07:12:56.85 +68:41:01.4
146.91382 27.07190 galactic Cam Second-epoch detections are separated by 1.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:12:56.85 +68:41:01.4 (user input) | T | P | (position from user input) J-Ks=0.584+/-0.027 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:56.85 +68:41:01.4: 13.11 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:56.85 +68:41:01.4: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.96 07:42:02.95 +69:30:29.5
146.08621 29.69451 galactic Cam Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:42:02.95 +69:30:29.5 (user input) | T | P | (position from user input) J-Ks=0.590+/-0.032 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:42:02.95 +69:30:29.5: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:42:02.95 +69:30:29.5: 13.12 +/- 0.02 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,2461258.8057,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.84 07:28:25.71 +70:15:29.3
145.23116 28.52183 galactic Cam Second-epoch detections are separated by 1.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:28:25.71 +70:15:29.3 (user input) | T | P | (position from user input) J-Ks=0.655+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:28:25.71 +70:15:29.3: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:28:25.71 +70:15:29.3: 13.13 +/- 0.02 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,2461258.8057,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.91 07:13:12.26 +69:06:50.9
146.43507 27.13644 galactic Cam Second-epoch detections are separated by 2.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:13:12.26 +69:06:50.9 (user input) | T | P | (position from user input) J-Ks=0.489+/-0.027 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:13:12.26 +69:06:50.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:13:12.26 +69:06:50.9: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 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,2461258.8057,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.91 07:23:31.53 +69:41:38.4
145.85493 28.08279 galactic Cam Second-epoch detections are separated by 1.3" and 5.7 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 | 07:23:31.53 +69:41:38.4 (user input) | T | P | (position from user input) J-Ks=0.287+/-0.028 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:23:31.53 +69:41:38.4: 13.11 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:23:31.53 +69:41:38.4: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.98 07:51:40.73 +70:05:38.0
145.36284 30.49581 galactic Cam Second-epoch detections are separated by 1.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:51:40.73 +70:05:38.0 (user input) | T | P | (position from user input) J-Ks=0.626+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:51:40.73 +70:05:38.0: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:51:40.73 +70:05:38.0: 13.12 +/- 0.02 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,2461258.8057,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 12.03 07:14:16.22 +68:53:47.3
146.68865 27.21128 galactic Cam Second-epoch detections are separated by 2.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:14:16.22 +68:53:47.3 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.025 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:14:16.22 +68:53:47.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:14:16.22 +68:53:47.3: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 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,2461258.8057,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.02 07:31:52.23 +70:11:36.1
145.31007 28.81192 galactic Cam Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:31:52.23 +70:11:36.1 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.029 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:31:52.23 +70:11:36.1: 13.08 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:31:52.23 +70:11:36.1: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.00 07:10:49.16 +69:03:26.9
146.47470 26.91903 galactic Cam Second-epoch detections are separated by 2.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:10:49.16 +69:03:26.9 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:10:49.16 +69:03:26.9: 13.08 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:10:49.16 +69:03:26.9: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.87 07:19:05.29 +68:47:59.5
146.83755 27.63643 galactic Cam Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:19:05.29 +68:47:59.5 (user input) | T | P | (position from user input) J-Ks=0.601+/-0.031 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:19:05.29 +68:47:59.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:19:05.29 +68:47:59.5: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.88 07:10:34.32 +69:08:33.3
146.37719 26.90596 galactic Cam Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:10:34.32 +69:08:33.3 (user input) | T | P | (position from user input) J-Ks=0.267+/-0.030 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:10:34.32 +69:08:33.3: 13.05 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:10:34.32 +69:08:33.3: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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,2461258.8057,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.93 07:12:37.64 +69:14:20.2
146.29003 27.09720 galactic Cam Second-epoch detections are separated by 1.3" and 5.9 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 | 07:12:37.64 +69:14:20.2 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.030 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:37.64 +69:14:20.2: 13.06 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:37.64 +69:14:20.2: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.96 07:05:36.84 +68:27:36.5
147.07674 26.38097 galactic Cam Second-epoch detections are separated by 1.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:05:36.84 +68:27:36.5 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.027 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:05:36.84 +68:27:36.5: 13.05 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:05:36.84 +68:27:36.5: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 12.01 07:45:01.61 +70:12:41.6
145.26546 29.92526 galactic Cam Second-epoch detections are separated by 1.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:45:01.61 +70:12:41.6 (user input) | T | P | (position from user input) J-Ks=0.662+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:45:01.61 +70:12:41.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:45:01.61 +70:12:41.6: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.98 07:27:13.18 +69:16:24.3
146.34725 28.38859 galactic Cam Second-epoch detections are separated by 1.0" and 5.7 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 | 07:27:13.18 +69:16:24.3 (user input) | T | P | (position from user input) J-Ks=0.450+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:27:13.18 +69:16:24.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:27:13.18 +69:16:24.3: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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,2461258.8057,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.93 06:50:22.94 +67:50:41.8
147.49540 24.88328 galactic Cam Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:50:22.94 +67:50:41.8 (user input) | T | P | (position from user input) J-Ks=0.272+/-0.033 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:50:22.94 +67:50:41.8: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:50:22.94 +67:50:41.8: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.94 07:38:46.17 +69:50:37.7
145.70752 29.40262 galactic Cam Second-epoch detections are separated by 2.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:38:46.17 +69:50:37.7 (user input) | T | P | (position from user input) J-Ks=0.620+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:38:46.17 +69:50:37.7: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:38:46.17 +69:50:37.7: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.96 07:05:14.38 +68:24:21.4
147.13169 26.33978 galactic Cam Second-epoch detections are separated by 1.5" and 5.9 pix
The object was found in VSX 1" Gaia DR3 1103081574532359168
Type: ROT
# Max. Min./Amp. JD0 Period
12.780 G 12.820 G K
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:05:14.38 +68:24:21.4: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:05:14.38 +68:24:21.4: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 1103081574532359168,2461258.8057,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103081574532359168 20260806.3057 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.96 07:32:24.75 +69:11:44.5
146.44946 28.84667 galactic Cam Second-epoch detections are separated by 1.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:32:24.75 +69:11:44.5 (user input) | T | P | (position from user input) J-Ks=0.188+/-0.030 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:32:24.75 +69:11:44.5: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:32:24.75 +69:11:44.5: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.91 07:05:22.33 +67:49:29.6
147.77588 26.27422 galactic Cam Second-epoch detections are separated by 3.0" and 6.1 pix
The object was found in VSX 6" Gaia DR3 1103039518212774016
Type: ROT
# Max. Min./Amp. JD0 Period
16.820 G 16.870 G 1.655530000000 K
ATTENTION: measured mag 11.91 is 4.9 mag brighter than the VSX record maximum brightness 16.82 - 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_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:05:22.33 +67:49:29.6: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:05:22.33 +67:49:29.6: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1103039518212774016,2461258.8057,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103039518212774016 20260806.3057 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 08 06.3057 2461258.8057 11.92 08:00:48.29 +71:04:00.7
144.15024 31.15718 galactic Cam Second-epoch detections are separated by 2.2" and 5.9 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 | 08:00:48.29 +71:04:00.7 (user input) | T | P | (position from user input) J-Ks=0.270+/-0.026 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 08:00:48.29 +71:04:00.7: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 08:00:48.29 +71:04:00.7: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 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,2461258.8057,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.84 07:33:09.72 +70:11:16.3
145.31710 28.92131 galactic Cam Second-epoch detections are separated by 1.2" and 5.7 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 | 07:33:09.72 +70:11:16.3 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:33:09.72 +70:11:16.3: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:33:09.72 +70:11:16.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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,2461258.8057,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.87 07:20:35.25 +69:19:32.2
146.25530 27.80582 galactic Cam Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:20:35.25 +69:19:32.2 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.032 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:35.25 +69:19:32.2: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:35.25 +69:19:32.2: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.87 07:00:49.76 +68:35:40.3
146.86085 25.96595 galactic Cam Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:00:49.76 +68:35:40.3 (user input) | T | P | (position from user input) J-Ks=0.496+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:00:49.76 +68:35:40.3: 13.02 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:00:49.76 +68:35:40.3: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.94 07:26:53.20 +69:36:59.2
145.95643 28.37152 galactic Cam Second-epoch detections are separated by 1.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:26:53.20 +69:36:59.2 (user input) | T | P | (position from user input) J-Ks=0.599+/-0.031 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:53.20 +69:36:59.2: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:53.20 +69:36:59.2: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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
target,2461258.8057,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.94 07:21:12.26 +69:51:47.7
145.65188 27.89115 galactic Cam Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:21:12.26 +69:51:47.7 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.032 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:12.26 +69:51:47.7: 12.98 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:12.26 +69:51:47.7: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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,2461258.8057,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.99 07:01:32.57 +67:50:03.9
147.70766 25.91807 galactic Cam Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:01:32.57 +67:50:03.9 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.036 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:01:32.57 +67:50:03.9: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:01:32.57 +67:50:03.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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
target,2461258.8057,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.85 07:18:04.47 +68:30:24.4
147.15924 27.52196 galactic Cam Second-epoch detections are separated by 2.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:18:04.47 +68:30:24.4 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:04.47 +68:30:24.4: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:04.47 +68:30:24.4: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 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,2461258.8057,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.82 07:37:20.61 +70:05:24.9
145.42688 29.27691 galactic Cam Second-epoch detections are separated by 1.1" and 5.9 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 | 07:37:20.61 +70:05:24.9 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:37:20.61 +70:05:24.9: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:37:20.61 +70:05:24.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 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,2461258.8057,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.78 07:15:00.85 +69:10:10.3
146.38938 27.30188 galactic Cam Second-epoch detections are separated by 0.1" and 5.7 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 | 07:15:00.85 +69:10:10.3 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.032 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:15:00.85 +69:10:10.3: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:15:00.85 +69:10:10.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.94 07:42:51.67 +70:09:15.2
145.34017 29.74421 galactic Cam Second-epoch detections are separated by 2.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:42:51.67 +70:09:15.2 (user input) | T | P | (position from user input) J-Ks=0.689+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:42:51.67 +70:09:15.2: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:42:51.67 +70:09:15.2: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 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,2461258.8057,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.89 07:01:19.99 +68:34:29.6
146.88995 26.00857 galactic Cam Second-epoch detections are separated by 1.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:01:19.99 +68:34:29.6 (user input) | T | P | (position from user input) J-Ks=0.608+/-0.031 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:01:19.99 +68:34:29.6: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:01:19.99 +68:34:29.6: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.92 07:32:47.31 +69:15:22.5
146.38089 28.88091 galactic Cam Second-epoch detections are separated by 1.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:32:47.31 +69:15:22.5 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.033 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:32:47.31 +69:15:22.5: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:32:47.31 +69:15:22.5: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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,2461258.8057,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.88 07:06:36.77 +67:58:40.6
147.62393 26.41023 galactic Cam Second-epoch detections are separated by 1.4" and 5.5 pix
The object was found in VSX 1" Gaia DR3 1103018730571033344
Type: ROT
# Max. Min./Amp. JD0 Period
12.700 G 12.720 G 24.683000000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:06:36.77 +67:58:40.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:06:36.77 +67:58:40.6: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1103018730571033344,2461258.8057,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103018730571033344 20260806.3057 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.87 07:19:31.74 +68:54:38.3
146.71604 27.68406 galactic Cam Second-epoch detections are separated by 2.3" and 5.9 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 | 07:19:31.74 +68:54:38.3 (user input) | T | P | (position from user input) J-Ks=0.750+/-0.027 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:19:31.74 +68:54:38.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:19:31.74 +68:54:38.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 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,2461258.8057,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.77 07:15:16.49 +69:15:43.0
146.28797 27.33281 galactic Cam Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:15:16.49 +69:15:43.0 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:15:16.49 +69:15:43.0: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:15:16.49 +69:15:43.0: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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,2461258.8057,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.86 07:38:07.17 +70:11:47.8
145.30379 29.34121 galactic Cam Second-epoch detections are separated by 2.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:38:07.17 +70:11:47.8 (user input) | T | P | (position from user input) J-Ks=0.289+/-0.027 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:38:07.17 +70:11:47.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:38:07.17 +70:11:47.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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,2461258.8057,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.87 07:24:31.04 +68:52:04.5
146.79521 28.12979 galactic Cam Second-epoch detections are separated by 1.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:24:31.04 +68:52:04.5 (user input) | T | P | (position from user input) J-Ks=0.625+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:24:31.04 +68:52:04.5: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:24:31.04 +68:52:04.5: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.88 07:56:32.17 +70:28:04.7
144.88931 30.87258 galactic Cam Second-epoch detections are separated by 3.6" and 6.3 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 | 07:56:32.17 +70:28:04.7 (user input) | T | P | (position from user input) J-Ks=0.728+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:56:32.17 +70:28:04.7: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:56:32.17 +70:28:04.7: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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,2461258.8057,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.88 07:02:59.89 +68:51:41.8
146.59760 26.19859 galactic Cam Second-epoch detections are separated by 0.3" and 5.7 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 | 07:02:59.89 +68:51:41.8 (user input) | T | P | (position from user input) J-Ks=0.617+/-0.031 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:02:59.89 +68:51:41.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:02:59.89 +68:51:41.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 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
target,2461258.8057,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.84 07:55:42.65 +70:47:35.4
144.52005 30.77318 galactic Cam Second-epoch detections are separated by 1.0" and 5.7 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 | 07:55:42.65 +70:47:35.4 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.033 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:55:42.65 +70:47:35.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:55:42.65 +70:47:35.4: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 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
target,2461258.8057,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.89 07:24:46.09 +69:10:48.8
146.44268 28.16753 galactic Cam Second-epoch detections are separated by 1.6" and 5.5 pix
The object was found in VSX 1" Gaia DR3 1108758078186406528
Type: ROT
# Max. Min./Amp. JD0 Period
12.570 G 12.660 G K
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:24:46.09 +69:10:48.8: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:24:46.09 +69:10:48.8: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 1108758078186406528,2461258.8057,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108758078186406528 20260806.3057 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.81 06:51:23.11 +67:50:46.2
147.51408 24.97630 galactic Cam Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:51:23.11 +67:50:46.2 (user input) | T | P | (position from user input) J-Ks=0.571+/-0.032 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:51:23.11 +67:50:46.2: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:51:23.11 +67:50:46.2: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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,2461258.8057,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.90 07:23:42.13 +69:09:33.0
146.46123 28.07184 galactic Cam Second-epoch detections are separated by 1.8" and 5.9 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 | 07:23:42.13 +69:09:33.0 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:23:42.13 +69:09:33.0: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:23:42.13 +69:09:33.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 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,2461258.8057,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.86 07:24:38.85 +69:28:29.8
146.10816 28.17044 galactic Cam Second-epoch detections are separated by 1.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:24:38.85 +69:28:29.8 (user input) | T | P | (position from user input) J-Ks=0.322+/-0.033 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:24:38.85 +69:28:29.8: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:24:38.85 +69:28:29.8: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 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,2461258.8057,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.85 06:47:54.29 +67:49:00.1
147.47478 24.64861 galactic Cam Second-epoch detections are separated by 1.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:47:54.29 +67:49:00.1 (user input) | T | P | (position from user input) J-Ks=0.452+/-0.032 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:47:54.29 +67:49:00.1: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:47:54.29 +67:49:00.1: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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,2461258.8057,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.89 07:44:52.41 +70:02:49.3
145.45578 29.91958 galactic Cam Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:44:52.41 +70:02:49.3 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:44:52.41 +70:02:49.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:44:52.41 +70:02:49.3: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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,2461258.8057,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.73 07:28:29.01 +70:17:57.9
145.18431 28.52737 galactic Cam Second-epoch detections are separated by 0.9" and 5.6 pix
The object was found in VSX 1" Gaia DR3 1108936954984017024
Type: ROT
# Max. Min./Amp. JD0 Period
12.550 G 12.590 G K
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:28:29.01 +70:17:57.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:28:29.01 +70:17:57.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 1108936954984017024,2461258.8057,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108936954984017024 20260806.3057 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.89 06:58:11.14 +68:38:04.2
146.77616 25.73386 galactic Cam Second-epoch detections are separated by 0.4" and 5.7 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 | 06:58:11.14 +68:38:04.2 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.026 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:58:11.14 +68:38:04.2: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:58:11.14 +68:38:04.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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,2461258.8057,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.82 07:54:58.91 +70:56:17.9
144.35859 30.69987 galactic Cam Second-epoch detections are separated by 0.6" and 5.9 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 | 07:54:58.91 +70:56:17.9 (user input) | T | P | (position from user input) J-Ks=0.627+/-0.031 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:54:58.91 +70:56:17.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:54:58.91 +70:56:17.9: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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,2461258.8057,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.79 07:38:36.42 +69:26:06.2
146.17686 29.39419 galactic Cam Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:38:36.42 +69:26:06.2 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:38:36.42 +69:26:06.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:38:36.42 +69:26:06.2: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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,2461258.8057,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.86 07:16:56.86 +69:45:49.6
145.73736 27.51831 galactic Cam Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:16:56.86 +69:45:49.6 (user input) | T | P | (position from user input) J-Ks=0.778+/-0.027 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:16:56.86 +69:45:49.6: 12.83 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:16:56.86 +69:45:49.6: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.80 07:12:04.83 +68:49:23.9
146.74908 27.00771 galactic Cam Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:12:04.83 +68:49:23.9 (user input) | T | P | (position from user input) J-Ks=0.300+/-0.030 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:04.83 +68:49:23.9: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:04.83 +68:49:23.9: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.87 07:32:33.46 +69:38:25.7
145.94187 28.86545 galactic Cam Second-epoch detections are separated by 1.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108692691604417408 | 07:32:33.39 +69:38:26.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.678+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:32:33.46 +69:38:25.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:32:33.46 +69:38:25.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1108692691604417408,2461258.8057,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108692691604417408 20260806.3057 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 08 06.3057 2461258.8057 11.84 07:03:55.84 +68:32:36.8
146.96168 26.23918 galactic Cam Second-epoch detections are separated by 2.9" and 5.5 pix
The object was found in VSX 1" Gaia DR3 1103095662025101056
Type: ROT
# Max. Min./Amp. JD0 Period
12.620 G 12.640 G 13.768000000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:03:55.84 +68:32:36.8: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:03:55.84 +68:32:36.8: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1103095662025101056,2461258.8057,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103095662025101056 20260806.3057 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.71 07:31:13.74 +69:47:28.7
145.76803 28.75229 galactic Cam Second-epoch detections are separated by 0.8" and 5.7 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 | 07:31:13.74 +69:47:28.7 (user input) | T | P | (position from user input) J-Ks=0.544+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:31:13.74 +69:47:28.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:31:13.74 +69:47:28.7: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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,2461258.8057,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.75 07:15:24.28 +69:02:49.3
146.53011 27.32601 galactic Cam Second-epoch detections are separated by 0.8" and 5.9 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 | 07:15:24.28 +69:02:49.3 (user input) | T | P | (position from user input) J-Ks=0.472+/-0.026 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:15:24.28 +69:02:49.3: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:15:24.28 +69:02:49.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461258.8057,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.76 07:51:14.18 +70:48:26.0
144.54091 30.40548 galactic Cam Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:51:14.18 +70:48:26.0 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.034 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:51:14.18 +70:48:26.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:51:14.18 +70:48:26.0: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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,2461258.8057,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.80 07:16:21.43 +69:45:23.2
145.74132 27.46683 galactic Cam Second-epoch detections are separated by 1.1" and 5.7 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 | Large-amplitude variable Gaia DR2 1109587762787741056 | 07:16:21.43 +69:45:23.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.634+/-0.026 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:16:21.43 +69:45:23.2: 12.81 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:16:21.43 +69:45:23.2: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1109587762787741056,2461258.8057,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1109587762787741056 20260806.3057 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 08 06.3057 2461258.8057 11.82 07:07:09.56 +68:17:39.4
147.28073 26.50103 galactic Cam Second-epoch detections are separated by 1.0" and 5.7 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 | 07:07:09.56 +68:17:39.4 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:07:09.56 +68:17:39.4: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:07:09.56 +68:17:39.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461258.8057,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.83 07:03:20.79 +68:51:23.6
146.60794 26.22902 galactic Cam Second-epoch detections are separated by 1.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:03:20.79 +68:51:23.6 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.031 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:03:20.79 +68:51:23.6: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:03:20.79 +68:51:23.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.71 07:25:33.65 +69:58:40.8
145.54137 28.26993 galactic Cam Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:25:33.65 +69:58:40.8 (user input) | T | P | (position from user input) J-Ks=0.598+/-0.027 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:25:33.65 +69:58:40.8: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:25:33.65 +69:58:40.8: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.88 07:18:17.71 +69:21:20.7
146.20602 27.60611 galactic Cam Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:18:17.71 +69:21:20.7 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.029 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:17.71 +69:21:20.7: 12.80 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:17.71 +69:21:20.7: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461258.8057,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.84 07:08:54.07 +68:27:37.8
147.11792 26.68042 galactic Cam Second-epoch detections are separated by 0.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1109042817339571968 | 07:08:54.01 +68:27:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.599+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:08:54.07 +68:27:37.8: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:08:54.07 +68:27:37.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 1109042817339571968,2461258.8057,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109042817339571968 20260806.3057 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.85 07:24:11.97 +69:46:46.7
145.76095 28.14499 galactic Cam Second-epoch detections are separated by 2.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:24:11.97 +69:46:46.7 (user input) | T | P | (position from user input) J-Ks=0.331+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:24:11.97 +69:46:46.7: 12.80 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:24:11.97 +69:46:46.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 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 08 06.3057 2461258.8057 11.77 07:21:13.88 +68:54:04.7
146.73821 27.83626 galactic Cam Second-epoch detections are separated by 0.5" and 5.7 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 | 07:21:13.88 +68:54:04.7 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.031 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:13.88 +68:54:04.7: 12.79 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:13.88 +68:54:04.7: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.72 07:31:15.47 +69:55:49.9
145.60928 28.75677 galactic Cam Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108907646127296384 | 07:31:15.24 +69:55:49.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.623+/-0.029 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:31:15.47 +69:55:49.9: 12.78 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:31:15.47 +69:55:49.9: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1108907646127296384,2461258.8057,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108907646127296384 20260806.3057 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.81 07:20:06.48 +69:03:59.2
146.54449 27.74655 galactic Cam Second-epoch detections are separated by 1.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108427434424690304 | 07:20:06.58 +69:03:59.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.637+/-0.026 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:06.48 +69:03:59.2: 12.78 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:06.48 +69:03:59.2: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 1108427434424690304,2461258.8057,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108427434424690304 20260806.3057 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.77 07:17:56.25 +69:55:49.4
145.55666 27.61510 galactic Cam Second-epoch detections are separated by 1.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1109611436647867520 | 07:18:03.36 +69:56:01.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1941BHarO.915...10G BD+70 444 J-Ks=0.514+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:17:56.25 +69:55:49.4: 12.74 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:17:56.25 +69:55:49.4: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1109611436647867520,2461258.8057,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109611436647867520 20260806.3057 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.82 08:01:22.23 +71:09:08.3
144.04459 31.19221 galactic Cam Second-epoch detections are separated by 0.6" and 6.0 pix
The object was found in VSX22" Gaia DR3 1098662706017563648
Type: ROT
# Max. Min./Amp. JD0 Period
15.390 G 15.430 G G
ATTENTION: measured mag 11.82 is 3.6 mag brighter than the VSX record maximum brightness 15.39 - 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_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 08:01:22.23 +71:09:08.3: 12.79 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 08:01:22.23 +71:09:08.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 1098662706017563648,2461258.8057,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1098662706017563648 20260806.3057 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.71 07:20:12.63 +69:37:34.0
145.91393 27.79146 galactic Cam Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108830542874529408 | 07:20:12.65 +69:37:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.686+/-0.027 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:12.63 +69:37:34.0: 12.76 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:12.63 +69:37:34.0: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1108830542874529408,2461258.8057,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108830542874529408 20260806.3057 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.82 07:18:28.44 +69:01:46.0
146.57456 27.59824 galactic Cam Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108433687897088128 | 07:18:28.56 +69:01:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.913+/-0.027 (M)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:28.44 +69:01:46.0: 12.77 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:28.44 +69:01:46.0: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 1108433687897088128,2461258.8057,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108433687897088128 20260806.3057 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.74 07:26:57.92 +69:38:46.3
145.92290 28.37937 galactic Cam Second-epoch detections are separated by 1.5" and 5.7 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 | Large-amplitude variable Gaia DR2 1108794774386937600 | 07:26:57.92 +69:38:46.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.609+/-0.032 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:57.92 +69:38:46.3: 12.76 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:57.92 +69:38:46.3: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1108794774386937600,2461258.8057,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1108794774386937600 20260806.3057 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.78 07:49:58.51 +70:50:27.8
144.51083 30.29967 galactic Cam Second-epoch detections are separated by 1.3" and 5.9 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 1110324298140077312 | 07:49:58.61 +70:50:27.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.736+/-0.032 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:49:58.51 +70:50:27.8: 12.77 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:49:58.51 +70:50:27.8: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 1110324298140077312,2461258.8057,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110324298140077312 20260806.3057 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.80 07:00:56.07 +68:31:01.3
146.94768 25.96403 galactic Cam Second-epoch detections are separated by 2.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1103279585404913920 | 07:00:55.99 +68:31:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.781+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:00:56.07 +68:31:01.3: 12.75 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:00:56.07 +68:31:01.3: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1103279585404913920,2461258.8057,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103279585404913920 20260806.3057 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 08 06.3057 2461258.8057 11.76 07:20:15.80 +69:59:00.0
145.51111 27.81731 galactic Cam Second-epoch detections are separated by 1.5" and 5.9 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 | 07:20:15.80 +69:59:00.0 (user input) | T | P | (position from user input) J-Ks=0.287+/-0.028 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:15.80 +69:59:00.0: 12.75 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:15.80 +69:59:00.0: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.77 06:59:18.89 +68:30:40.6
146.92915 25.81655 galactic Cam Second-epoch detections are separated by 0.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:59:18.89 +68:30:40.6 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:59:18.89 +68:30:40.6: 12.76 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:59:18.89 +68:30:40.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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,2461258.8057,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.81 07:28:36.82 +69:21:04.4
146.26344 28.51422 galactic Cam Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1108775636010619008 | 07:28:36.82 +69:21:04.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.335+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:28:36.82 +69:21:04.4: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:28:36.82 +69:21:04.4: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1108775636010619008,2461258.8057,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1108775636010619008 20260806.3057 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.76 07:12:56.85 +69:08:25.5
146.40325 27.11615 galactic Cam Second-epoch detections are separated by 1.4" and 5.7 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 | 07:12:56.85 +69:08:25.5 (user input) | T | P | (position from user input) J-Ks=0.307+/-0.028 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:56.85 +69:08:25.5: 12.74 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:56.85 +69:08:25.5: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.74 07:40:20.28 +70:57:34.0
144.42289 29.50618 galactic Cam Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:40:20.28 +70:57:34.0 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:40:20.28 +70:57:34.0: 12.74 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:40:20.28 +70:57:34.0: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.73 07:45:09.50 +70:46:39.3
144.61258 29.90856 galactic Cam Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:45:09.50 +70:46:39.3 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.028 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:45:09.50 +70:46:39.3: 12.72 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:45:09.50 +70:46:39.3: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.82 07:01:39.70 +67:34:55.6
147.98680 25.89093 galactic Cam Second-epoch detections are separated by 2.0" and 5.9 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 J105.4249+67.5808 | 07:01:39.70 +67:34:55.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.593+/-0.032 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:01:39.70 +67:34:55.6: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:01:39.70 +67:34:55.6: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.4249+67.5808,2461258.8057,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J105.4249+67.5808 20260806.3057 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.73 07:47:20.20 +70:59:07.8
144.36106 30.07466 galactic Cam Second-epoch detections are separated by 1.2" and 5.9 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 1110340236761644032 | 07:47:20.05 +70:59:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.583+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:47:20.20 +70:59:07.8: 12.73 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:47:20.20 +70:59:07.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1110340236761644032,2461258.8057,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110340236761644032 20260806.3057 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.78 07:11:14.70 +68:52:52.7
146.67567 26.93870 galactic Cam Second-epoch detections are separated by 2.2" and 5.7 pix
The object was found in VSX 2" Gaia DR3 1109076867840107648
Type: ROT
# Max. Min./Amp. JD0 Period
12.800 G 12.840 G G
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:11:14.70 +68:52:52.7: 12.72 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:11:14.70 +68:52:52.7: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1109076867840107648,2461258.8057,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109076867840107648 20260806.3057 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.80 07:37:45.49 +69:50:39.7
145.70830 29.31550 galactic Cam Second-epoch detections are separated by 1.2" and 5.8 pix
The object was found in VSX 2" Gaia DR3 1110208059145622144
Type: ROT
# Max. Min./Amp. JD0 Period
12.430 G 12.460 G K
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:37:45.49 +69:50:39.7: 12.71 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:37:45.49 +69:50:39.7: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1110208059145622144,2461258.8057,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110208059145622144 20260806.3057 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 08 06.3057 2461258.8057 11.75 07:40:32.80 +70:45:07.3
144.66047 29.53016 galactic Cam Second-epoch detections are separated by 2.1" and 5.6 pix
The object was found in VSX 1" NSVS 683300
Type: EW
# Max. Min./Amp. JD0 Period
12.823 g Y 0.428 g 2458204.72450 0.679649800000
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:40:32.80 +70:45:07.3: 12.71 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:40:32.80 +70:45:07.3: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 683300,2461258.8057,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 683300 20260806.3057 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.71 07:37:23.16 +70:46:07.2
144.64918 29.26944 galactic Cam Second-epoch detections are separated by 0.9" and 5.9 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 1110276160146883712 | 07:37:23.14 +70:46:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.803+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:37:23.16 +70:46:07.2: 12.71 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:37:23.16 +70:46:07.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1110276160146883712,2461258.8057,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110276160146883712 20260806.3057 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.70 07:21:02.82 +68:48:47.0
146.83657 27.81396 galactic Cam Second-epoch detections are separated by 1.6" and 5.7 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 | 07:21:02.82 +68:48:47.0 (user input) | T | P | (position from user input) J-Ks=0.796+/-0.029 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:02.82 +68:48:47.0: 12.71 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:02.82 +68:48:47.0: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.64 07:14:43.77 +69:41:59.0
145.79242 27.32180 galactic Cam Second-epoch detections are separated by 1.2" and 5.8 pix
The object was found in VSX 1" Gaia DR3 1109592641871079040
Type: ROT
# Max. Min./Amp. JD0 Period
12.490 G 12.510 G G
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:14:43.77 +69:41:59.0: 12.69 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:14:43.77 +69:41:59.0: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1109592641871079040,2461258.8057,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109592641871079040 20260806.3057 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.78 07:52:25.44 +71:01:40.1
144.27675 30.48432 galactic Cam Second-epoch detections are separated by 1.6" and 5.9 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 1098692427191328640 | 07:52:25.41 +71:01:40.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.671+/-0.032 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:52:25.44 +71:01:40.1: 12.70 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:52:25.44 +71:01:40.1: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1098692427191328640,2461258.8057,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1098692427191328640 20260806.3057 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.73 07:46:31.52 +70:42:00.2
144.69485 30.02535 galactic Cam Second-epoch detections are separated by 2.8" and 6.2 pix
The object was found in VSX13" Gaia DR3 1110295539039205888
Type: ROT
# Max. Min./Amp. JD0 Period
17.530 G 17.610 G K
ATTENTION: measured mag 11.73 is 5.8 mag brighter than the VSX record maximum brightness 17.53 - 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_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:46:31.52 +70:42:00.2: 12.69 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:46:31.52 +70:42:00.2: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1110295539039205888,2461258.8057,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110295539039205888 20260806.3057 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.73 07:26:35.58 +69:32:09.5
146.04679 28.34306 galactic Cam Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:26:35.58 +69:32:09.5 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:35.58 +69:32:09.5: 12.67 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:35.58 +69:32:09.5: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 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,2461258.8057,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.75 07:00:26.92 +68:35:07.0
146.86530 25.93022 galactic Cam Second-epoch detections are separated by 1.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1103286599090953472 | 07:00:26.77 +68:35:06.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.452+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:00:26.92 +68:35:07.0: 12.67 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:00:26.92 +68:35:07.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1103286599090953472,2461258.8057,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103286599090953472 20260806.3057 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.60 07:29:49.08 +70:04:42.8
145.43832 28.63605 galactic Cam Second-epoch detections are separated by 1.2" and 5.7 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 1108913933959429760 | 07:29:48.87 +70:04:42.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.446+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:29:49.08 +70:04:42.8: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:29:49.08 +70:04:42.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1108913933959429760,2461258.8057,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108913933959429760 20260806.3057 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.76 07:21:27.01 +69:57:52.4
145.53871 27.91772 galactic Cam Second-epoch detections are separated by 0.4" and 5.7 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 1108865276273043840 | 07:21:26.94 +69:57:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.428+/-0.031 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:27.01 +69:57:52.4: 12.67 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:27.01 +69:57:52.4: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1108865276273043840,2461258.8057,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108865276273043840 20260806.3057 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.72 07:43:22.88 +70:28:54.4
144.96118 29.77522 galactic Cam Second-epoch detections are separated by 0.7" and 5.7 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 1110297257026153088 | 07:43:22.87 +70:28:54.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.361+/-0.028 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:43:22.88 +70:28:54.4: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:43:22.88 +70:28:54.4: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1110297257026153088,2461258.8057,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110297257026153088 20260806.3057 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.67 06:32:38.27 +66:44:05.4
148.24292 22.96084 galactic Cam Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1104380265263822976 | 06:32:37.86 +66:44:03.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:32:38.27 +66:44:05.4: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:32:38.27 +66:44:05.4: 12.64 +/- 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
Gaia DR3 1104380265263822976,2461258.8057,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1104380265263822976 20260806.3057 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.74 07:32:12.40 +70:18:03.1
145.18761 28.84112 galactic Cam Second-epoch detections are separated by 2.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1110423352969076736 | 07:32:12.27 +70:18:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.434+/-0.029 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:32:12.40 +70:18:03.1: 12.65 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:32:12.40 +70:18:03.1: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 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 1110423352969076736,2461258.8057,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110423352969076736 20260806.3057 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.71 07:49:43.74 +71:09:47.2
144.14064 30.25592 galactic Cam Second-epoch detections are separated by 1.1" and 5.9 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 1110707340503245184 | 07:49:43.62 +71:09:47.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.030 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:49:43.74 +71:09:47.2: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:49:43.74 +71:09:47.2: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1110707340503245184,2461258.8057,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110707340503245184 20260806.3057 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.72 07:04:46.76 +68:40:48.6
146.82218 26.33408 galactic Cam Second-epoch detections are separated by 1.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1109102534564756736 | 07:04:46.76 +68:40:48.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.035 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:04:46.76 +68:40:48.6: 12.65 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:04:46.76 +68:40:48.6: 12.66 +/- 0.01 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
Gaia DR3 1109102534564756736,2461258.8057,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109102534564756736 20260806.3057 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.68 06:56:02.82 +68:03:33.8
147.36936 25.44502 galactic Cam Second-epoch detections are separated by 1.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1103163556866880896 | 06:56:02.82 +68:03:34.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.274+/-0.036 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:56:02.82 +68:03:33.8: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:56:02.82 +68:03:33.8: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1103163556866880896,2461258.8057,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103163556866880896 20260806.3057 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.68 07:33:34.86 +69:52:19.8
145.67800 28.95580 galactic Cam Second-epoch detections are separated by 0.3" and 5.7 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 | 07:33:34.86 +69:52:19.8 (user input) | T | P | (position from user input) J-Ks=0.266+/-0.030 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:33:34.86 +69:52:19.8: 12.65 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:33:34.86 +69:52:19.8: 12.73 +/- 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,2461258.8057,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.66 06:59:24.27 +67:41:53.4
147.82221 25.69705 galactic Cam Second-epoch detections are separated by 1.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1102950320329595904 | 06:59:24.22 +67:41:53.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.705+/-0.026 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:59:24.27 +67:41:53.4: 12.65 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:59:24.27 +67:41:53.4: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1102950320329595904,2461258.8057,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1102950320329595904 20260806.3057 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.70 07:14:29.80 +68:53:54.7
146.68844 27.23176 galactic Cam Second-epoch detections are separated by 2.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1109155409904365440 | 07:14:29.94 +68:53:54.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.025 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:14:29.80 +68:53:54.7: 12.64 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:14:29.80 +68:53:54.7: 12.66 +/- 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
Gaia DR3 1109155409904365440,2461258.8057,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109155409904365440 20260806.3057 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.62 07:13:08.88 +69:09:51.7
146.37835 27.13616 galactic Cam Second-epoch detections are separated by 1.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1109169119439967872 | 07:13:08.78 +69:09:51.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.608+/-0.025 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:13:08.88 +69:09:51.7: 12.64 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:13:08.88 +69:09:51.7: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 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 1109169119439967872,2461258.8057,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109169119439967872 20260806.3057 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.59 07:30:11.12 +70:04:13.8
145.44812 28.66720 galactic Cam Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108913693441256576 | 07:30:12.67 +70:03:39.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.031 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:30:11.12 +70:04:13.8: 12.63 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:30:11.12 +70:04:13.8: 12.63 +/- 0.01 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 1108913693441256576,2461258.8057,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108913693441256576 20260806.3057 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.66 07:21:11.04 +69:01:00.5
146.60755 27.83935 galactic Cam Second-epoch detections are separated by 0.6" and 5.9 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 1108425372837646080 | 07:21:06.74 +69:00:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.263+/-0.028 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:11.04 +69:01:00.5: 12.63 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:11.04 +69:01:00.5: 12.63 +/- 0.01 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 1108425372837646080,2461258.8057,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108425372837646080 20260806.3057 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.71 07:25:14.18 +69:32:35.2
146.03342 28.22487 galactic Cam Second-epoch detections are separated by 0.7" and 5.9 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 1108796178839237632 | 07:25:14.02 +69:32:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.568+/-0.026 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:25:14.18 +69:32:35.2: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:25:14.18 +69:32:35.2: 12.63 +/- 0.01 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 1108796178839237632,2461258.8057,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108796178839237632 20260806.3057 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.62 07:47:18.35 +70:29:00.4
144.94042 30.10252 galactic Cam Second-epoch detections are separated by 1.3" and 5.9 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 1110288701451267456 | 07:47:18.32 +70:29:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.297+/-0.032 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:47:18.35 +70:29:00.4: 12.63 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:47:18.35 +70:29:00.4: 12.65 +/- 0.01 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
Gaia DR3 1110288701451267456,2461258.8057,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110288701451267456 20260806.3057 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.71 07:52:15.54 +70:09:55.5
145.27582 30.53970 galactic Cam Second-epoch detections are separated by 1.9" and 5.8 pix
The object was found in VSX 2" Gaia DR3 1098257291167164160
Type: ROT
# Max. Min./Amp. JD0 Period
12.400 G 12.420 G K
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:52:15.54 +70:09:55.5: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:52:15.54 +70:09:55.5: 12.65 +/- 0.01 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 1098257291167164160,2461258.8057,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1098257291167164160 20260806.3057 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.67 07:53:34.49 +70:07:40.2
145.30925 30.65401 galactic Cam Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1098209466708365568 | 07:53:34.48 +70:07:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.598+/-0.035 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:53:34.49 +70:07:40.2: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:53:34.49 +70:07:40.2: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 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
Gaia DR3 1098209466708365568,2461258.8057,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1098209466708365568 20260806.3057 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.69 07:09:51.96 +68:53:48.7
146.64350 26.81689 galactic Cam Second-epoch detections are separated by 0.3" and 5.7 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 1109078448388081920 | 07:09:51.77 +68:53:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.539+/-0.029 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:09:51.96 +68:53:48.7: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:09:51.96 +68:53:48.7: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1109078448388081920,2461258.8057,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109078448388081920 20260806.3057 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.71 08:06:24.51 +71:24:54.0
143.67559 31.55701 galactic Cam Second-epoch detections are separated by 2.3" and 5.7 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 1098774753124056960 | 08:06:24.51 +71:24:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.789+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 08:06:24.51 +71:24:54.0: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 08:06:24.51 +71:24:54.0: 12.66 +/- 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 1098774753124056960,2461258.8057,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1098774753124056960 20260806.3057 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.54 07:29:38.86 +69:21:13.9
146.26332 28.60541 galactic Cam Second-epoch detections are separated by 0.9" and 5.6 pix
The object was found in VSX 0" ASASSN-V J072938.95+692113.9
Type: L
# Max. Min./Amp. JD0 Period
12.480 V 12.980 V
The object was not found in astcheck.
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:29:38.86 +69:21:13.9: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:29:38.86 +69:21:13.9: 12.81 +/- 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
ASASSN-V J072938.95+692113.9,2461258.8057,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J072938.95+692113.9 20260806.3057 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 08 06.3057 2461258.8057 11.67 07:08:28.53 +68:28:28.5
147.09713 26.64329 galactic Cam Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:08:28.53 +68:28:28.5 (user input) | T | P | (position from user input) J-Ks=0.576+/-0.039 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:08:28.53 +68:28:28.5: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:08:28.53 +68:28:28.5: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8057,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.65 07:34:41.64 +69:41:54.1
145.87709 29.05138 galactic Cam Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:34:41.64 +69:41:54.1 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:34:41.64 +69:41:54.1: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:34:41.64 +69:41:54.1: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 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,2461258.8057,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.66 07:27:14.99 +69:29:51.9
146.09250 28.39914 galactic Cam Second-epoch detections are separated by 0.8" and 5.9 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 | 07:27:14.99 +69:29:51.9 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.026 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:27:14.99 +69:29:51.9: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:27:14.99 +69:29:51.9: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 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
target,2461258.8057,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.3057 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.69 06:59:03.24 +68:34:15.1
146.85967 25.80217 galactic Cam Second-epoch detections are separated by 0.9" and 5.7 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 1103284327049176576 | 06:59:03.25 +68:34:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.609+/-0.029 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:59:03.24 +68:34:15.1: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:59:03.24 +68:34:15.1: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1103284327049176576,2461258.8057,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103284327049176576 20260806.3057 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.68 07:51:30.71 +70:06:02.4
145.35618 30.48115 galactic Cam Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1098255401381917184 | 07:51:30.65 +70:06:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.369+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:51:30.71 +70:06:02.4: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:51:30.71 +70:06:02.4: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1098255401381917184,2461258.8057,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1098255401381917184 20260806.3057 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.68 07:41:33.28 +70:58:55.4
144.39277 29.60447 galactic Cam Second-epoch detections are separated by 0.5" and 5.7 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 1110365044492745344 | 07:41:33.23 +70:58:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.639+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:41:33.28 +70:58:55.4: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:41:33.28 +70:58:55.4: 12.67 +/- 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 1110365044492745344,2461258.8057,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110365044492745344 20260806.3057 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.65 07:18:01.45 +69:06:09.0
146.48900 27.56360 galactic Cam Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108434924847671552 | 07:18:01.33 +69:06:08.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=11.005+/- (unrealisitic color!)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:01.45 +69:06:09.0: 12.59 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:01.45 +69:06:09.0: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 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
Gaia DR3 1108434924847671552,2461258.8057,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108434924847671552 20260806.3057 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.63 07:09:02.18 +68:38:37.3
146.91584 26.71391 galactic Cam Second-epoch detections are separated by 0.9" and 5.9 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 1109068965100562688 | 07:09:02.12 +68:38:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.602+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:09:02.18 +68:38:37.3: 12.59 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:09:02.18 +68:38:37.3: 12.62 +/- 0.01 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 1109068965100562688,2461258.8057,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109068965100562688 20260806.3057 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 08 06.3057 2461258.8057 11.68 06:53:48.70 +68:17:09.0
147.08263 25.27973 galactic Cam Second-epoch detections are separated by 0.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1103218154491035648 | 06:53:48.49 +68:17:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.425+/-0.034 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:53:48.70 +68:17:09.0: 12.58 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:53:48.70 +68:17:09.0: 12.61 +/- 0.01 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 1103218154491035648,2461258.8057,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103218154491035648 20260806.3057 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.65 07:33:57.63 +69:22:08.1
146.25346 28.98564 galactic Cam Second-epoch detections are separated by 0.9" and 5.7 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 1108673102256080640 | 07:33:57.67 +69:22:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.031 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:33:57.63 +69:22:08.1: 12.59 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:33:57.63 +69:22:08.1: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 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
Gaia DR3 1108673102256080640,2461258.8057,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108673102256080640 20260806.3057 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.68 06:58:34.80 +68:01:58.6
147.44170 25.67413 galactic Cam Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1103151737116854400 | 06:58:34.63 +68:01:58.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.453+/-0.024 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:58:34.80 +68:01:58.6: 12.58 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:58:34.80 +68:01:58.6: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 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
Large-amplitude variable Gaia DR2 1103151737116854400,2461258.8057,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1103151737116854400 20260806.3057 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.60 07:05:20.19 +68:24:13.3
147.13548 26.34831 galactic Cam Second-epoch detections are separated by 0.4" and 5.7 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 1103081505812880128 | 07:05:20.22 +68:24:12.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.031 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:05:20.19 +68:24:13.3: 12.58 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:05:20.19 +68:24:13.3: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1103081505812880128,2461258.8057,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1103081505812880128 20260806.3057 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.64 07:46:21.87 +70:12:43.5
145.25851 30.03831 galactic Cam Second-epoch detections are separated by 2.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1110278359170066432 | 07:46:21.74 +70:12:44.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.661+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:46:21.87 +70:12:43.5: 12.57 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:46:21.87 +70:12:43.5: 12.61 +/- 0.01 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 1110278359170066432,2461258.8057,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110278359170066432 20260806.3057 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.61 07:07:17.32 +68:33:42.2
146.98576 26.54591 galactic Cam Second-epoch detections are separated by 2.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1109091054113927424 | 07:07:17.19 +68:33:41.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.747+/-0.033 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:07:17.32 +68:33:42.2: 12.56 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:07:17.32 +68:33:42.2: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 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 1109091054113927424,2461258.8057,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1109091054113927424 20260806.3057 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 08 06.3057 2461258.8057 11.61 07:44:46.41 +70:58:43.7
144.38270 29.86659 galactic Cam Second-epoch detections are separated by 1.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1110338587494203008 | 07:44:46.29 +70:58:43.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.401+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:44:46.41 +70:58:43.7: 12.55 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:44:46.41 +70:58:43.7: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 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 1110338587494203008,2461258.8057,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1110338587494203008 20260806.3057 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 08 06.3057 2461258.8057 11.64 07:35:13.42 +69:25:02.4
146.19874 29.09704 galactic Cam Second-epoch detections are separated by 1.5" and 5.7 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 1108671766523727360 | 07:35:13.39 +69:25:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.670+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:35:13.42 +69:25:02.4: 12.54 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:35:13.42 +69:25:02.4: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1108671766523727360,2461258.8057,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108671766523727360 20260806.3057 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.59 07:28:29.01 +69:38:20.1
145.93580 28.51112 galactic Cam Second-epoch detections are separated by 0.6" and 5.9 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 1108876859802378496 | 07:28:29.04 +69:38:20.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.664+/-0.029 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:28:29.01 +69:38:20.1: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:28:29.01 +69:38:20.1: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1108876859802378496,2461258.8057,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108876859802378496 20260806.3057 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.58 07:26:07.47 +70:11:17.3
145.30472 28.32511 galactic Cam Second-epoch detections are separated by 1.7" and 5.7 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 1108953065404540416 | 07:26:07.29 +70:11:17.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.468+/-0.030 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:07.47 +70:11:17.3: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:07.47 +70:11:17.3: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1108953065404540416,2461258.8057,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108953065404540416 20260806.3057 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.51 07:22:59.98 +69:52:43.9
145.64322 28.04621 galactic Cam Second-epoch detections are separated by 1.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108851399235948032 | 07:22:59.99 +69:52:43.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.432+/-0.027 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:22:59.98 +69:52:43.9: 12.43 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:22:59.98 +69:52:43.9: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1108851399235948032,2461258.8057,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108851399235948032 20260806.3057 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.46 07:29:08.52 +70:26:35.0
145.02203 28.58545 galactic Cam Second-epoch detections are separated by 0.4" and 5.7 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 1108939699466306048 | 07:29:08.42 +70:26:35.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.346+/-0.030 (G)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:29:08.52 +70:26:35.0: 12.40 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:29:08.52 +70:26:35.0: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1108939699466306048,2461258.8057,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108939699466306048 20260806.3057 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.41 07:19:59.13 +69:33:17.0
145.99309 27.76745 galactic Cam Second-epoch detections are separated by 0.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108828511352663040 | 07:19:59.18 +69:33:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.651+/-0.028 (K)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:19:59.13 +69:33:17.0: 12.36 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:19:59.13 +69:33:17.0: 12.41 +/- 0.01 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 1108828511352663040,2461258.8057,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108828511352663040 20260806.3057 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3057 2461258.8057 11.41 07:29:04.65 +69:54:00.8
145.63992 28.56906 galactic Cam Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1108887575742920448 | 07:29:04.62 +69:54:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.312+/-0.027 (F)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:29:04.65 +69:54:00.8: 12.32 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:29:04.65 +69:54:00.8: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1108887575742920448,2461258.8057,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1108887575742920448 20260806.3057 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.79056218 18.01.2026 06:58:14.572 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
First image: 2461058.79056218 18.01.2026 06:58:14.572 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Last image: 2461258.80596603 06.08.2026 07:20:25.465 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 3 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): 8651
Objects passed selection criteria: 8584
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: 4948.25
Average stars matched: 4845.5 (97.9235 %)
Memory usage VmPeak: 235896 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:43:35 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: 2461058.79056218 18.01.2026 06:58:14.572 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
First image: 2461058.79056218 18.01.2026 06:58:14.572 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Last image: 2461258.80596603 06.08.2026 07:20:25.465 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 166
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.16
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: 9 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): 57977
Objects passed selection criteria: 57766
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: 34676.2
Average stars matched: 33362.2 (96.2107 %)
Memory usage VmPeak: 283576 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:44:13 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/TTUQ2b1x1/TTUQ2_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/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
SExtractor catalog cache: saved Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.cat to cache
SExtractor catalog cache: saved Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.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/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.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: 2461258.80534640
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_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits exists and is non-empty
Saving wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits to local_wcs_cache/
'wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits' -> 'local_wcs_cache/wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits'
wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits exists and is non-empty
Saving wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits to local_wcs_cache/
'wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits' -> 'local_wcs_cache/wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits'
wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits exists and is non-empty
Saving wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits to local_wcs_cache/
'wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits' -> 'local_wcs_cache/wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits'
wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits exists and is non-empty
Saving wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits to local_wcs_cache/
'wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits' -> 'local_wcs_cache/wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits (1st reference image)
verification OK: wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Image size: 941.7'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: 07:12:16.597 +69:59:23.56 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_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits (1st new image)
verification OK: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
Image size: 938.2'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 07:12:07.684 +69:58:11.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:12:16.597 +69:59:23.56
Second-epoch image center 07:12:07.684 +69:58:11.59
Angular distance between the image centers 0.0237 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits (2nd new image)
verification OK: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Image size: 938.3'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 07:12:09.318 +69:58:44.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:12:16.597 +69:59:23.56
Second-epoch image center 07:12:09.318 +69:58:44.36
Angular distance between the image centers 0.0150 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 07:12:07.684 +69:58:11.59
Second-epoch second image center 07:12:09.318 +69:58:44.36
Angular distance between the image centers 0.00940 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/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits &> /tmp/tmp.OM6IzKhm7O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits &> /tmp/tmp.HfgE8ggBHG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits &> /tmp/tmp.578li1ddcB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits &> /tmp/tmp.0AtNzJOLAE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.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_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits and wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.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_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits and wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat
Found non-empty wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits and wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat
The reference image (wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits) and catalog (wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat) found
'wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat' -> 'wcsmag.cat'
Read 13381 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.6278 to 136.5003 deg, Dec +62.8981 to +75.4711 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 80.6278 to 136.5003 deg, Dec 62.8981 to 75.4711 deg
Loaded 12882 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): 7117 out of 7564 total matches.
Matched with Tycho-2 7564 out of 13381 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.875800
a=0.000000 b=1.000000 c=22.875800
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 13381 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.6278 to 136.5003 deg, Dec +62.8981 to +75.4711 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 80.6278 to 136.5003 deg, Dec 62.8981 to 75.4711 deg
Loaded 12882 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): 7117 out of 7564 total matches.
Matched with Tycho-2 7564 out of 13381 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Forced-photometry filter: calibrated wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits -> calib.txt_param_ref_wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits (aperture=6.1)
Read 12112 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.6280 to 136.5006 deg, Dec +62.8981 to +75.4817 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 80.6280 to 136.5006 deg, Dec 62.8981 to 75.4817 deg
Loaded 12888 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): 7048 out of 7472 total matches.
Matched with Tycho-2 7472 out of 12112 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
Forced-photometry filter: calibrated wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits -> calib.txt_param_ref_wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
2.2 pix Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
2.2 pix fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
2.2 pix fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Limiting magnitude estimates:
15.4 mag. Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
15.2 mag. Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
11.7 mag. fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
11.8 mag. fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
All-image limiting magnitude estimate: 11.7 (SNR ) 9.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OM6IzKhm7O (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/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits' -> 'wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.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/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
WCS_IMAGE_NAME=wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
WCS-calibrated image found: wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Checking if the catalog wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat corresponding to the image wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits alredy exist and is non-empty...
Catalog wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat corresponding to the image wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
WCS catalog name: wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=962, bad_region=3723, passed=13381
Got 13381 stars (including 8954 good ones) from the SExtractor catalog wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat
util/solve_plate_with_UCAC5 got 13381 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 10466 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 10466 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 10466 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4887 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits N_match=4887 sigma_overall_arcsec=0.277 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.258 sigma_q3_arcsec=0.268 sigma_q4_arcsec=0.236 n_q1=1474 n_q2=962 n_q3=1441 n_q4=1010 worst_quadrant_to_overall_ratio=1.287
The image catalog is written to wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits -region wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.HfgE8ggBHG (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/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits' -> 'wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.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/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
WCS-calibrated image found: wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
Checking if the catalog wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
WCS catalog name: wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=905, bad_region=3431, passed=12112
Got 12112 stars (including 8027 good ones) from the SExtractor catalog wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat
util/solve_plate_with_UCAC5 got 12112 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 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 4889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 9427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 9427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 9427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4888 stars left (next iteration limit 5376)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits N_match=4888 sigma_overall_arcsec=0.406 sigma_q1_arcsec=0.516 sigma_q2_arcsec=0.371 sigma_q3_arcsec=0.375 sigma_q4_arcsec=0.361 n_q1=1480 n_q2=967 n_q3=1431 n_q4=1010 worst_quadrant_to_overall_ratio=1.272
The image catalog is written to wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits -region wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.578li1ddcB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
WCS_IMAGE_NAME=wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
WCS-calibrated image found: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
Checking if the catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat corresponding to the image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat corresponding to the image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
WCS catalog name: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=39, bad_region=246, passed=1009
Got 1009 stars (including 739 good ones) from the SExtractor catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat
util/solve_plate_with_UCAC5 got 1009 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 766 to 827 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 707 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 703 matched stars entering correct_measured_positions(), 683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 703 matched stars entering correct_measured_positions(), 766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 766 to 827 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 708 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 704 matched stars entering correct_measured_positions(), 765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 704 matched stars entering correct_measured_positions(), 766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 704 stars left (next iteration limit 773)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=704 robust_rms=6.693 arcsec worst_quadrant_rms=7.664 arcsec
SIP_REFIT: SIP order 3 trial: matched=704 robust_rms=0.783 arcsec worst_quadrant_rms=0.917 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=704 robust_rms_before=1.377 arcsec robust_rms_before_corrected=0.607 arcsec robust_rms_after=0.783 arcsec worst_quadrant_rms_before=0.741 worst_quadrant_rms_after=0.917
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.741 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits N_match=704 sigma_overall_arcsec=0.628 sigma_q1_arcsec=0.639 sigma_q2_arcsec=0.583 sigma_q3_arcsec=0.717 sigma_q4_arcsec=0.600 n_q1=272 n_q2=157 n_q3=153 n_q4=122 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits -region wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0AtNzJOLAE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
WCS_IMAGE_NAME=wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
WCS-calibrated image found: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Checking if the catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat corresponding to the image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat corresponding to the image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
WCS catalog name: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=58, bad_region=242, passed=1042
Got 1042 stars (including 756 good ones) from the SExtractor catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat
util/solve_plate_with_UCAC5 got 1042 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 726 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 722 matched stars entering correct_measured_positions(), 708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 722 matched stars entering correct_measured_positions(), 810 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 726 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 721 matched stars entering correct_measured_positions(), 808 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 721 matched stars entering correct_measured_positions(), 808 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 721 stars left (next iteration limit 794)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=721 robust_rms=7.109 arcsec worst_quadrant_rms=9.074 arcsec
SIP_REFIT: SIP order 3 trial: matched=721 robust_rms=0.771 arcsec worst_quadrant_rms=1.000 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=721 robust_rms_before=1.368 arcsec robust_rms_before_corrected=0.605 arcsec robust_rms_after=0.771 arcsec worst_quadrant_rms_before=0.764 worst_quadrant_rms_after=1.000
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.764 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits N_match=721 sigma_overall_arcsec=0.622 sigma_q1_arcsec=0.520 sigma_q2_arcsec=0.586 sigma_q3_arcsec=0.735 sigma_q4_arcsec=0.672 n_q1=291 n_q2=147 n_q3=161 n_q4=122 worst_quadrant_to_overall_ratio=1.182
The image catalog is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits -region wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits sigma_overall=0.277 worst_q_ratio=1.287
ref2=Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits sigma_overall=0.406 worst_q_ratio=1.272
new1=fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits sigma_overall=0.628 worst_q_ratio=1.142
new2=fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits sigma_overall=0.622 worst_q_ratio=1.182
reference average sigma_overall=0.3415 worst_q_ratio=1.2795
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286_astrometric_residuals.png (4887 matched stars from wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290_astrometric_residuals.png (4888 matched stars from wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306_astrometric_residuals.png (704 matched stars from wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.59 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307_astrometric_residuals.png (721 matched stars from wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits'
Saving fully-calibrated image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits'
Preparing the HTML report for the field Cam-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cam-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
SExtractor catalog cache: saved Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.cat to cache
SExtractor catalog cache: saved Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Creating symlink local_wcs_cache/wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits exists and is non-empty
wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits exists and is non-empty
wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits exists and is non-empty
wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits (1st reference image)
verification OK: wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Image size: 941.7'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: 07:12:16.597 +69:59:23.56 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_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits (1st new image)
verification OK: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
Image size: 938.2'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 07:12:07.684 +69:58:11.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:12:16.597 +69:59:23.56
Second-epoch image center 07:12:07.684 +69:58:11.59
Angular distance between the image centers 0.0237 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits (2nd new image)
verification OK: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Image size: 938.3'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 07:12:09.318 +69:58:44.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:12:16.597 +69:59:23.56
Second-epoch image center 07:12:09.318 +69:58:44.36
Angular distance between the image centers 0.0150 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 07:12:07.684 +69:58:11.59
Second-epoch second image center 07:12:09.318 +69:58:44.36
Angular distance between the image centers 0.00940 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/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits &> /tmp/tmp.F7Hz3mY50S
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits &> /tmp/tmp.HhAWyiYRZz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits &> /tmp/tmp.qlf09xFn50
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits &> /tmp/tmp.hAwpo8bIs3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.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_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits and wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.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_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits and wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat
Found non-empty wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits and wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat
The reference image (wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits) and catalog (wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat) found
'wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat' -> 'wcsmag.cat'
Read 82728 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.6278 to 136.5003 deg, Dec +62.8263 to +75.4768 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 80.6278 to 136.5003 deg, Dec 62.8263 to 75.4768 deg
Loaded 12989 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): 6445 out of 7627 total matches.
Matched with Tycho-2 7627 out of 82728 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.743500
a=0.000000 b=1.000000 c=22.743500
From vast_summary.log: estimated ref. image limiting mag.: -7.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 82728 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.6278 to 136.5003 deg, Dec +62.8263 to +75.4768 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 80.6278 to 136.5003 deg, Dec 62.8263 to 75.4768 deg
Loaded 12989 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): 6445 out of 7627 total matches.
Matched with Tycho-2 7627 out of 82728 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Forced-photometry filter: calibrated wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits -> calib.txt_param_ref_wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits (aperture=4.6)
Read 78594 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.6281 to 136.5004 deg, Dec +62.8266 to +75.4919 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 80.6281 to 136.5004 deg, Dec 62.8266 to 75.4919 deg
Loaded 13001 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): 6483 out of 7620 total matches.
Matched with Tycho-2 7620 out of 78594 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
Forced-photometry filter: calibrated wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits -> calib.txt_param_ref_wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 162 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
2.0 pix Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
1.9 pix fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
1.9 pix fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Limiting magnitude estimates:
15.6 mag. Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
15.5 mag. Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
12.2 mag. fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
12.2 mag. fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 12.2 (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.F7Hz3mY50S (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/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits' -> 'wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.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/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
WCS_IMAGE_NAME=wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
WCS-calibrated image found: wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
Checking if the catalog wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat corresponding to the image wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits alredy exist and is non-empty...
Catalog wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat corresponding to the image wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits
WCS catalog name: wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=11, blended=5466, bad_region=19090, passed=82717
Got 82717 stars (including 59431 good ones) from the SExtractor catalog wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat
util/solve_plate_with_UCAC5 got 82717 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 4890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 67595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 67595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 67595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4890 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits N_match=4890 sigma_overall_arcsec=0.268 sigma_q1_arcsec=0.329 sigma_q2_arcsec=0.250 sigma_q3_arcsec=0.255 sigma_q4_arcsec=0.222 n_q1=1485 n_q2=946 n_q3=1476 n_q4=983 worst_quadrant_to_overall_ratio=1.231
The image catalog is written to wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits -region wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.HhAWyiYRZz (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/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits' -> 'wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.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/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
WCS-calibrated image found: wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
Checking if the catalog wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits
WCS catalog name: wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=29, blended=5023, bad_region=18434, passed=78565
Got 78565 stars (including 56306 good ones) from the SExtractor catalog wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat
util/solve_plate_with_UCAC5 got 78565 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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 4888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 63890 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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 63890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 63890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4887 stars left (next iteration limit 5376)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits N_match=4887 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.482 sigma_q2_arcsec=0.364 sigma_q3_arcsec=0.367 sigma_q4_arcsec=0.331 n_q1=1471 n_q2=974 n_q3=1459 n_q4=983 worst_quadrant_to_overall_ratio=1.240
The image catalog is written to wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits -region wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qlf09xFn50 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
WCS_IMAGE_NAME=wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
WCS-calibrated image found: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
Checking if the catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat corresponding to the image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat corresponding to the image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
WCS catalog name: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=157, bad_region=2086, passed=9785
Got 9785 stars (including 7569 good ones) from the SExtractor catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat
util/solve_plate_with_UCAC5 got 9785 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 4861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 8207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 8207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 8207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 4860 stars left (next iteration limit 5346)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits N_match=4860 sigma_overall_arcsec=0.787 sigma_q1_arcsec=0.781 sigma_q2_arcsec=0.677 sigma_q3_arcsec=1.203 sigma_q4_arcsec=0.675 n_q1=1995 n_q2=1039 n_q3=988 n_q4=838 worst_quadrant_to_overall_ratio=1.529
The image catalog is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits -region wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hAwpo8bIs3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
WCS_IMAGE_NAME=wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
WCS-calibrated image found: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Checking if the catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat corresponding to the image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat corresponding to the image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
WCS catalog name: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=7, blended=187, bad_region=2096, passed=10056
Got 10056 stars (including 7821 good ones) from the SExtractor catalog wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat
util/solve_plate_with_UCAC5 got 10056 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 4866 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 4854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 8464 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 4867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 8464 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 8464 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 4854 stars left (next iteration limit 5338)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits N_match=4854 sigma_overall_arcsec=0.777 sigma_q1_arcsec=0.742 sigma_q2_arcsec=0.694 sigma_q3_arcsec=1.145 sigma_q4_arcsec=0.647 n_q1=2018 n_q2=1003 n_q3=1016 n_q4=817 worst_quadrant_to_overall_ratio=1.473
The image catalog is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits -region wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.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_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
Saving fully-calibrated image wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.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_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Preparing the HTML report for the field Cam-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:49:38.45 +67:46:49.0: 12.67 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:35:30.37 +66:49:57.7: 12.76 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:22:13.49 +69:43:12.2: 12.87 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:59:43.71 +68:29:44.9: 12.64 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:16:59.37 +68:23:57.3: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:13:53.42 +69:06:52.7: 12.78 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:16.39 +69:02:11.2: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:36:53.59 +69:19:06.4: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:27:10.47 +69:12:45.4: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:42:38.33 +69:52:50.6: 13.24 +/- 0.03 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:59:43.71 +68:29:44.9: 12.70 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:22:13.49 +69:43:12.2: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:13:53.42 +69:06:52.7: 12.85 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:49:38.45 +67:46:49.0: 12.67 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:35:30.37 +66:49:57.7: 12.78 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:36:53.59 +69:19:06.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:16.39 +69:02:11.2: 12.92 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:16:59.37 +68:23:57.3: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 06:59:43.71 +68:29:44.9: ref_mag=12.67 +/- 0.01 new_mean_mag=11.7277 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 07:22:13.49 +69:43:12.2: ref_mag=12.90 +/- 0.01 new_mean_mag=11.8157 delta=1.09 (need > 0.90)
Forced photometry filter KEPT candidate at 07:36:53.59 +69:19:06.4: ref_mag=12.85 +/- 0.01 new_mean_mag=11.7812 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 07:12:16.39 +69:02:11.2: ref_mag=12.91 +/- 0.01 new_mean_mag=11.8374 delta=1.08 (need > 0.90)
Forced photometry filter KEPT candidate at 07:13:53.42 +69:06:52.7: ref_mag=12.80 +/- 0.01 new_mean_mag=11.7102 delta=1.09 (need > 0.90)
Forced photometry filter KEPT candidate at 06:49:38.45 +67:46:49.0: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6603 delta=1.01 (need > 0.90)
Forced photometry filter KEPT candidate at 06:35:30.37 +66:49:57.7: ref_mag=12.77 +/- 0.01 new_mean_mag=11.7090 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 07:16:59.37 +68:23:57.3: ref_mag=12.97 +/- 0.01 new_mean_mag=11.9478 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:27:10.47 +69:12:45.4: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.01
Forced photometry filter KEPT candidate at 07:27:10.47 +69:12:45.4: ref_mag=13.11 +/- 0.01 new_mean_mag=11.8707 delta=1.23 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:42:38.33 +69:52:50.6: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 07:42:38.33 +69:52:50.6: ref_mag=13.27 +/- 0.02 new_mean_mag=12.0602 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:08:40.22 +68:28:15.2: 13.38 +/- 0.03 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:56:17.55 +67:04:48.4: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:08:40.22 +68:28:15.2: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:40.22 +68:28:15.2: ref_mag=13.41 +/- 0.02 new_mean_mag=12.1173 delta=1.29 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:56:17.55 +67:04:48.4: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 06:56:17.55 +67:04:48.4: ref_mag=13.25 +/- 0.02 new_mean_mag=12.0502 delta=1.20 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:10:50.86 +68:48:23.3: 13.44 +/- 0.03 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:31:17.48 +69:44:00.9: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:16.63 +69:27:16.0: 13.26 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:25:24.69 +69:55:46.4: 13.24 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:27:43.80 +70:22:54.8: 13.22 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:10:50.86 +68:48:23.3: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 07:10:50.86 +68:48:23.3: ref_mag=13.43 +/- 0.02 new_mean_mag=12.1013 delta=1.33 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:31:17.48 +69:44:00.9: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 07:31:17.48 +69:44:00.9: ref_mag=13.40 +/- 0.02 new_mean_mag=12.1203 delta=1.28 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:16.63 +69:27:16.0: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 07:18:16.63 +69:27:16.0: ref_mag=13.27 +/- 0.02 new_mean_mag=11.9542 delta=1.31 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:25:24.69 +69:55:46.4: 13.22 +/- 0.03 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:27:43.80 +70:22:54.8: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 07:25:24.69 +69:55:46.4: ref_mag=13.23 +/- 0.02 new_mean_mag=11.9994 delta=1.23 (need > 0.90)
Forced photometry filter KEPT candidate at 07:27:43.80 +70:22:54.8: ref_mag=13.23 +/- 0.02 new_mean_mag=12.0502 delta=1.18 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:19:03.99 +68:28:18.0: 13.22 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:19:03.99 +68:28:18.0: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 07:19:03.99 +68:28:18.0: ref_mag=13.23 +/- 0.02 new_mean_mag=11.9986 delta=1.23 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:36.83 +69:55:51.2: 13.18 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:31.55 +68:43:37.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:20.58 +69:39:57.1: 13.13 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:36.83 +69:55:51.2: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:56.85 +68:41:01.4: 13.11 +/- 0.02 detection
Forced photometry filter KEPT candidate at 07:26:36.83 +69:55:51.2: ref_mag=13.21 +/- 0.02 new_mean_mag=11.9962 delta=1.22 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:31.55 +68:43:37.1: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 07:12:31.55 +68:43:37.1: ref_mag=13.18 +/- 0.02 new_mean_mag=12.0369 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:20.58 +69:39:57.1: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 07:20:20.58 +69:39:57.1: ref_mag=13.13 +/- 0.02 new_mean_mag=11.9768 delta=1.16 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:56.85 +68:41:01.4: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 07:12:56.85 +68:41:01.4: ref_mag=13.13 +/- 0.02 new_mean_mag=11.9053 delta=1.22 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:42:02.95 +69:30:29.5: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:42:02.95 +69:30:29.5: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 07:42:02.95 +69:30:29.5: ref_mag=13.11 +/- 0.02 new_mean_mag=11.9646 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:28:25.71 +70:15:29.3: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:28:25.71 +70:15:29.3: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 07:28:25.71 +70:15:29.3: ref_mag=13.11 +/- 0.02 new_mean_mag=11.8394 delta=1.27 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:13:12.26 +69:06:50.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:13:12.26 +69:06:50.9: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry filter KEPT candidate at 07:13:12.26 +69:06:50.9: ref_mag=13.08 +/- 0.01 new_mean_mag=11.9055 delta=1.18 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:23:31.53 +69:41:38.4: 13.11 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:51:40.73 +70:05:38.0: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:23:31.53 +69:41:38.4: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry filter KEPT candidate at 07:23:31.53 +69:41:38.4: ref_mag=13.09 +/- 0.01 new_mean_mag=11.8869 delta=1.20 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:51:40.73 +70:05:38.0: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 07:51:40.73 +70:05:38.0: ref_mag=13.11 +/- 0.02 new_mean_mag=11.9729 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:14:16.22 +68:53:47.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:14:16.22 +68:53:47.3: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry filter KEPT candidate at 07:14:16.22 +68:53:47.3: ref_mag=13.08 +/- 0.01 new_mean_mag=12.0266 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:31:52.23 +70:11:36.1: 13.08 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:31:52.23 +70:11:36.1: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 07:31:52.23 +70:11:36.1: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0150 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:10:49.16 +69:03:26.9: 13.08 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:19:05.29 +68:47:59.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:10:34.32 +69:08:33.3: 13.05 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:19:05.29 +68:47:59.5: 13.09 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:10:49.16 +69:03:26.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:10:34.32 +69:08:33.3: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 07:19:05.29 +68:47:59.5: ref_mag=13.07 +/- 0.01 new_mean_mag=11.8600 delta=1.21 (need > 0.90)
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry filter KEPT candidate at 07:10:49.16 +69:03:26.9: ref_mag=13.09 +/- 0.01 new_mean_mag=11.9900 delta=1.10 (need > 0.90)
Forced photometry filter KEPT candidate at 07:10:34.32 +69:08:33.3: ref_mag=13.06 +/- 0.01 new_mean_mag=11.8913 delta=1.17 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:37.64 +69:14:20.2: 13.06 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:37.64 +69:14:20.2: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry filter KEPT candidate at 07:12:37.64 +69:14:20.2: ref_mag=13.09 +/- 0.01 new_mean_mag=11.9052 delta=1.19 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:05:36.84 +68:27:36.5: 13.05 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:05:36.84 +68:27:36.5: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 07:05:36.84 +68:27:36.5: ref_mag=13.07 +/- 0.01 new_mean_mag=11.9343 delta=1.13 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:45:01.61 +70:12:41.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:45:01.61 +70:12:41.6: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 07:45:01.61 +70:12:41.6: ref_mag=13.07 +/- 0.01 new_mean_mag=12.0007 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:27:13.18 +69:16:24.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:50:22.94 +67:50:41.8: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:27:13.18 +69:16:24.3: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.01
Forced photometry filter KEPT candidate at 07:27:13.18 +69:16:24.3: ref_mag=13.05 +/- 0.01 new_mean_mag=11.9455 delta=1.11 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:50:22.94 +67:50:41.8: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 06:50:22.94 +67:50:41.8: ref_mag=13.03 +/- 0.01 new_mean_mag=11.9252 delta=1.11 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:38:46.17 +69:50:37.7: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:05:14.38 +68:24:21.4: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:38:46.17 +69:50:37.7: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.01
Forced photometry filter KEPT candidate at 07:38:46.17 +69:50:37.7: ref_mag=13.04 +/- 0.01 new_mean_mag=11.9159 delta=1.12 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:05:14.38 +68:24:21.4: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 07:05:14.38 +68:24:21.4: ref_mag=13.02 +/- 0.01 new_mean_mag=11.9612 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:32:24.75 +69:11:44.5: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:05:22.33 +67:49:29.6: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 08:00:48.29 +71:04:00.7: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:32:24.75 +69:11:44.5: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 07:32:24.75 +69:11:44.5: ref_mag=13.03 +/- 0.01 new_mean_mag=11.9519 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:05:22.33 +67:49:29.6: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 07:05:22.33 +67:49:29.6: ref_mag=13.03 +/- 0.01 new_mean_mag=11.9145 delta=1.11 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 08:00:48.29 +71:04:00.7: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Forced photometry filter KEPT candidate at 08:00:48.29 +71:04:00.7: ref_mag=12.98 +/- 0.01 new_mean_mag=11.9184 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:33:09.72 +70:11:16.3: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:33:09.72 +70:11:16.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter KEPT candidate at 07:33:09.72 +70:11:16.3: ref_mag=12.99 +/- 0.01 new_mean_mag=11.8396 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:35.25 +69:19:32.2: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:35.25 +69:19:32.2: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 07:20:35.25 +69:19:32.2: ref_mag=13.03 +/- 0.01 new_mean_mag=11.8447 delta=1.18 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:00:49.76 +68:35:40.3: 13.02 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:00:49.76 +68:35:40.3: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 07:00:49.76 +68:35:40.3: ref_mag=13.04 +/- 0.02 new_mean_mag=11.8642 delta=1.18 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:53.20 +69:36:59.2: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:53.20 +69:36:59.2: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 07:26:53.20 +69:36:59.2: ref_mag=13.00 +/- 0.01 new_mean_mag=11.9428 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:12.26 +69:51:47.7: 12.98 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:12.26 +69:51:47.7: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 07:21:12.26 +69:51:47.7: ref_mag=13.02 +/- 0.01 new_mean_mag=11.9310 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:01:32.57 +67:50:03.9: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:04.47 +68:30:24.4: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:01:32.57 +67:50:03.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 07:01:32.57 +67:50:03.9: ref_mag=13.00 +/- 0.01 new_mean_mag=11.9833 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:04.47 +68:30:24.4: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Forced photometry filter KEPT candidate at 07:18:04.47 +68:30:24.4: ref_mag=13.01 +/- 0.01 new_mean_mag=11.8415 delta=1.17 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:37:20.61 +70:05:24.9: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:37:20.61 +70:05:24.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 07:37:20.61 +70:05:24.9: ref_mag=12.95 +/- 0.01 new_mean_mag=11.8236 delta=1.12 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:15:00.85 +69:10:10.3: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:15:00.85 +69:10:10.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 07:15:00.85 +69:10:10.3: ref_mag=12.96 +/- 0.01 new_mean_mag=11.7539 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:42:51.67 +70:09:15.2: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:01:19.99 +68:34:29.6: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:42:51.67 +70:09:15.2: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 07:42:51.67 +70:09:15.2: ref_mag=12.95 +/- 0.01 new_mean_mag=11.9148 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:01:19.99 +68:34:29.6: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 07:01:19.99 +68:34:29.6: ref_mag=12.96 +/- 0.01 new_mean_mag=11.8443 delta=1.12 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:32:47.31 +69:15:22.5: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:32:47.31 +69:15:22.5: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 07:32:47.31 +69:15:22.5: ref_mag=12.93 +/- 0.01 new_mean_mag=11.9191 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:06:36.77 +67:58:40.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:06:36.77 +67:58:40.6: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 07:06:36.77 +67:58:40.6: ref_mag=12.96 +/- 0.01 new_mean_mag=11.8511 delta=1.10 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:19:31.74 +68:54:38.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:19:31.74 +68:54:38.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 07:19:31.74 +68:54:38.3: ref_mag=12.95 +/- 0.01 new_mean_mag=11.8766 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:15:16.49 +69:15:43.0: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:15:16.49 +69:15:43.0: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 07:15:16.49 +69:15:43.0: ref_mag=12.90 +/- 0.01 new_mean_mag=11.7554 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:38:07.17 +70:11:47.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:38:07.17 +70:11:47.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 07:38:07.17 +70:11:47.8: ref_mag=12.90 +/- 0.01 new_mean_mag=11.8164 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:24:31.04 +68:52:04.5: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:24:31.04 +68:52:04.5: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 07:24:31.04 +68:52:04.5: ref_mag=12.88 +/- 0.01 new_mean_mag=11.8430 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:56:32.17 +70:28:04.7: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:56:32.17 +70:28:04.7: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 07:56:32.17 +70:28:04.7: ref_mag=12.93 +/- 0.01 new_mean_mag=11.8717 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:02:59.89 +68:51:41.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:51:23.11 +67:50:46.2: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:55:42.65 +70:47:35.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:24:46.09 +69:10:48.8: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:23:42.13 +69:09:33.0: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:24:38.85 +69:28:29.8: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:47:54.29 +67:49:00.1: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:24:38.85 +69:28:29.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:24:46.09 +69:10:48.8: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:02:59.89 +68:51:41.8: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:51:23.11 +67:50:46.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:55:42.65 +70:47:35.4: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:23:42.13 +69:09:33.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:47:54.29 +67:49:00.1: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 07:24:38.85 +69:28:29.8: ref_mag=12.89 +/- 0.01 new_mean_mag=11.8519 delta=1.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 07:24:46.09 +69:10:48.8: ref_mag=12.87 +/- 0.01 new_mean_mag=11.8790 delta=0.99 (need > 0.90)
Forced photometry filter KEPT candidate at 07:02:59.89 +68:51:41.8: ref_mag=12.91 +/- 0.01 new_mean_mag=11.8770 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 06:51:23.11 +67:50:46.2: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8183 delta=1.05 (need > 0.90)
Forced photometry filter KEPT candidate at 07:55:42.65 +70:47:35.4: ref_mag=12.92 +/- 0.01 new_mean_mag=11.7992 delta=1.12 (need > 0.90)
Forced photometry filter KEPT candidate at 06:47:54.29 +67:49:00.1: ref_mag=12.93 +/- 0.01 new_mean_mag=11.8424 delta=1.09 (need > 0.90)
Forced photometry filter KEPT candidate at 07:23:42.13 +69:09:33.0: ref_mag=12.89 +/- 0.01 new_mean_mag=11.8660 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:44:52.41 +70:02:49.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:44:52.41 +70:02:49.3: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 07:44:52.41 +70:02:49.3: ref_mag=12.85 +/- 0.01 new_mean_mag=11.8399 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:28:29.01 +70:17:57.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:28:29.01 +70:17:57.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 07:28:29.01 +70:17:57.9: ref_mag=12.87 +/- 0.01 new_mean_mag=11.7290 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:58:11.14 +68:38:04.2: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:54:58.91 +70:56:17.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:58:11.14 +68:38:04.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 06:58:11.14 +68:38:04.2: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8679 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:54:58.91 +70:56:17.9: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 07:54:58.91 +70:56:17.9: ref_mag=12.84 +/- 0.01 new_mean_mag=11.8194 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:38:36.42 +69:26:06.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:38:36.42 +69:26:06.2: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 07:38:36.42 +69:26:06.2: ref_mag=12.86 +/- 0.01 new_mean_mag=11.7848 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:16:56.86 +69:45:49.6: 12.83 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:04.83 +68:49:23.9: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:03:55.84 +68:32:36.8: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:32:33.46 +69:38:25.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:31:13.74 +69:47:28.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:15:24.28 +69:02:49.3: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:32:33.46 +69:38:25.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 07:32:33.46 +69:38:25.7: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8582 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:51:14.18 +70:48:26.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:04.83 +68:49:23.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:31:13.74 +69:47:28.7: 12.89 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:16:56.86 +69:45:49.6: 12.83 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:03:55.84 +68:32:36.8: 12.85 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:15:24.28 +69:02:49.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 07:12:04.83 +68:49:23.9: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8051 delta=1.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 07:16:56.86 +69:45:49.6: ref_mag=12.83 +/- 0.01 new_mean_mag=11.7861 delta=1.05 (need > 0.90)
Forced photometry filter KEPT candidate at 07:31:13.74 +69:47:28.7: ref_mag=12.85 +/- 0.01 new_mean_mag=11.7070 delta=1.14 (need > 0.90)
Forced photometry filter KEPT candidate at 07:03:55.84 +68:32:36.8: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8345 delta=1.00 (need > 0.90)
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 07:15:24.28 +69:02:49.3: ref_mag=12.82 +/- 0.01 new_mean_mag=11.7460 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:51:14.18 +70:48:26.0: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 07:51:14.18 +70:48:26.0: ref_mag=12.84 +/- 0.01 new_mean_mag=11.7468 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:16:21.43 +69:45:23.2: 12.81 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:16:21.43 +69:45:23.2: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 07:16:21.43 +69:45:23.2: ref_mag=12.82 +/- 0.01 new_mean_mag=11.7748 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:07:09.56 +68:17:39.4: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:03:20.79 +68:51:23.6: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:07:09.56 +68:17:39.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 07:07:09.56 +68:17:39.4: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8221 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:03:20.79 +68:51:23.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 07:03:20.79 +68:51:23.6: ref_mag=12.81 +/- 0.01 new_mean_mag=11.8345 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:25:33.65 +69:58:40.8: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:25:33.65 +69:58:40.8: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 07:25:33.65 +69:58:40.8: ref_mag=12.81 +/- 0.01 new_mean_mag=11.7266 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:17.71 +69:21:20.7: 12.80 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:08:54.07 +68:27:37.8: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:24:11.97 +69:46:46.7: 12.80 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:13.88 +68:54:04.7: 12.79 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:17.71 +69:21:20.7: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 07:18:17.71 +69:21:20.7: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8850 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:08:54.07 +68:27:37.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 07:08:54.07 +68:27:37.8: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8327 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:24:11.97 +69:46:46.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 07:24:11.97 +69:46:46.7: ref_mag=12.81 +/- 0.01 new_mean_mag=11.8429 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:13.88 +68:54:04.7: 12.85 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:31:15.47 +69:55:49.9: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 07:21:13.88 +68:54:04.7: ref_mag=12.81 +/- 0.01 new_mean_mag=11.7466 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:31:15.47 +69:55:49.9: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 07:31:15.47 +69:55:49.9: ref_mag=12.81 +/- 0.01 new_mean_mag=11.7232 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:06.48 +69:03:59.2: 12.78 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:06.48 +69:03:59.2: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 07:20:06.48 +69:03:59.2: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8056 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:17:56.25 +69:55:49.4: 12.74 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:17:56.25 +69:55:49.4: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter KEPT candidate at 07:17:56.25 +69:55:49.4: ref_mag=12.74 +/- 0.01 new_mean_mag=11.7111 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 08:01:22.23 +71:09:08.3: 12.79 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:12.63 +69:37:34.0: 12.76 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 08:01:22.23 +71:09:08.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 08:01:22.23 +71:09:08.3: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8093 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:28.44 +69:01:46.0: 12.77 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:12.63 +69:37:34.0: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 07:20:12.63 +69:37:34.0: ref_mag=12.76 +/- 0.01 new_mean_mag=11.6927 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:28.44 +69:01:46.0: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 07:18:28.44 +69:01:46.0: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8176 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:57.92 +69:38:46.3: 12.76 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:57.92 +69:38:46.3: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 07:26:57.92 +69:38:46.3: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7381 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:49:58.51 +70:50:27.8: 12.77 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:00:56.07 +68:31:01.3: 12.75 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:20:15.80 +69:59:00.0: 12.75 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:49:58.51 +70:50:27.8: 12.78 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:00:56.07 +68:31:01.3: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 07:49:58.51 +70:50:27.8: ref_mag=12.77 +/- 0.01 new_mean_mag=11.7739 delta=1.00 (need > 0.90)
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 07:00:56.07 +68:31:01.3: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7945 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:20:15.80 +69:59:00.0: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 07:20:15.80 +69:59:00.0: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7427 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:59:18.89 +68:30:40.6: 12.76 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:59:18.89 +68:30:40.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 06:59:18.89 +68:30:40.6: ref_mag=12.77 +/- 0.01 new_mean_mag=11.7696 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:28:36.82 +69:21:04.4: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:28:36.82 +69:21:04.4: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 07:28:36.82 +69:21:04.4: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7993 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:12:56.85 +69:08:25.5: 12.74 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:40:20.28 +70:57:34.0: 12.74 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:40:20.28 +70:57:34.0: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:12:56.85 +69:08:25.5: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter KEPT candidate at 07:12:56.85 +69:08:25.5: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7540 delta=1.00 (need > 0.90)
Forced photometry filter KEPT candidate at 07:40:20.28 +70:57:34.0: ref_mag=12.74 +/- 0.01 new_mean_mag=11.7434 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:45:09.50 +70:46:39.3: 12.72 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:45:09.50 +70:46:39.3: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 07:45:09.50 +70:46:39.3: ref_mag=12.73 +/- 0.01 new_mean_mag=11.7203 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:01:39.70 +67:34:55.6: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:01:39.70 +67:34:55.6: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 07:01:39.70 +67:34:55.6: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7706 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:47:20.20 +70:59:07.8: 12.73 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:47:20.20 +70:59:07.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 07:47:20.20 +70:59:07.8: ref_mag=12.75 +/- 0.01 new_mean_mag=11.6717 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:11:14.70 +68:52:52.7: 12.72 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:37:45.49 +69:50:39.7: 12.71 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:11:14.70 +68:52:52.7: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 07:11:14.70 +68:52:52.7: ref_mag=12.73 +/- 0.01 new_mean_mag=11.7802 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:37:45.49 +69:50:39.7: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter KEPT candidate at 07:37:45.49 +69:50:39.7: ref_mag=12.74 +/- 0.01 new_mean_mag=11.7980 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:40:32.80 +70:45:07.3: 12.71 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:37:23.16 +70:46:07.2: 12.71 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:02.82 +68:48:47.0: 12.71 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:40:32.80 +70:45:07.3: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 07:40:32.80 +70:45:07.3: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7414 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:37:23.16 +70:46:07.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 07:37:23.16 +70:46:07.2: ref_mag=12.71 +/- 0.01 new_mean_mag=11.6861 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:02.82 +68:48:47.0: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 07:21:02.82 +68:48:47.0: ref_mag=12.72 +/- 0.01 new_mean_mag=11.7019 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:14:43.77 +69:41:59.0: 12.69 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:14:43.77 +69:41:59.0: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 07:14:43.77 +69:41:59.0: ref_mag=12.69 +/- 0.01 new_mean_mag=11.6371 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:52:25.44 +71:01:40.1: 12.70 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:35.58 +69:32:09.5: 12.67 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:46:31.52 +70:42:00.2: 12.69 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:46:31.52 +70:42:00.2: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:52:25.44 +71:01:40.1: 12.72 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:35.58 +69:32:09.5: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 07:46:31.52 +70:42:00.2: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7324 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 07:52:25.44 +71:01:40.1: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7395 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 07:26:35.58 +69:32:09.5: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7306 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:00:26.92 +68:35:07.0: 12.67 +/- 0.02 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:00:26.92 +68:35:07.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 07:00:26.92 +68:35:07.0: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7502 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:29:49.08 +70:04:42.8: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:29:49.08 +70:04:42.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 07:29:49.08 +70:04:42.8: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6014 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:27.01 +69:57:52.4: 12.67 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:27.01 +69:57:52.4: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 07:21:27.01 +69:57:52.4: ref_mag=12.69 +/- 0.01 new_mean_mag=11.7562 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:43:22.88 +70:28:54.4: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:43:22.88 +70:28:54.4: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 07:43:22.88 +70:28:54.4: ref_mag=12.67 +/- 0.01 new_mean_mag=11.7239 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:32:38.27 +66:44:05.4: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:32:38.27 +66:44:05.4: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 06:32:38.27 +66:44:05.4: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6692 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:32:12.40 +70:18:03.1: 12.65 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:32:12.40 +70:18:03.1: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 07:32:12.40 +70:18:03.1: ref_mag=12.66 +/- 0.01 new_mean_mag=11.7264 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:49:43.74 +71:09:47.2: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:04:46.76 +68:40:48.6: 12.65 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:49:43.74 +71:09:47.2: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 07:49:43.74 +71:09:47.2: ref_mag=12.67 +/- 0.01 new_mean_mag=11.7081 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:04:46.76 +68:40:48.6: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 07:04:46.76 +68:40:48.6: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6980 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:56:02.82 +68:03:33.8: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:33:34.86 +69:52:19.8: 12.65 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:59:24.27 +67:41:53.4: 12.65 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:56:02.82 +68:03:33.8: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 06:56:02.82 +68:03:33.8: ref_mag=12.69 +/- 0.01 new_mean_mag=11.6834 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:33:34.86 +69:52:19.8: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 07:33:34.86 +69:52:19.8: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6791 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:59:24.27 +67:41:53.4: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 06:59:24.27 +67:41:53.4: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6617 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:14:29.80 +68:53:54.7: 12.64 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:13:08.88 +69:09:51.7: 12.64 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:14:29.80 +68:53:54.7: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 07:14:29.80 +68:53:54.7: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6955 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:13:08.88 +69:09:51.7: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 07:13:08.88 +69:09:51.7: ref_mag=12.66 +/- 0.01 new_mean_mag=11.6251 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:30:11.12 +70:04:13.8: 12.63 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:30:11.12 +70:04:13.8: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 07:30:11.12 +70:04:13.8: ref_mag=12.63 +/- 0.01 new_mean_mag=11.5968 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:21:11.04 +69:01:00.5: 12.63 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:21:11.04 +69:01:00.5: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 07:21:11.04 +69:01:00.5: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6483 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:25:14.18 +69:32:35.2: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:25:14.18 +69:32:35.2: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 07:25:14.18 +69:32:35.2: ref_mag=12.63 +/- 0.01 new_mean_mag=11.7065 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:47:18.35 +70:29:00.4: 12.63 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:52:15.54 +70:09:55.5: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:47:18.35 +70:29:00.4: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 07:47:18.35 +70:29:00.4: ref_mag=12.64 +/- 0.01 new_mean_mag=11.6351 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:52:15.54 +70:09:55.5: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 07:52:15.54 +70:09:55.5: ref_mag=12.63 +/- 0.01 new_mean_mag=11.7000 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:53:34.49 +70:07:40.2: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:09:51.96 +68:53:48.7: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 08:06:24.51 +71:24:54.0: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:53:34.49 +70:07:40.2: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 07:53:34.49 +70:07:40.2: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6577 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:09:51.96 +68:53:48.7: 12.63 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 08:06:24.51 +71:24:54.0: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 07:09:51.96 +68:53:48.7: ref_mag=12.62 +/- 0.01 new_mean_mag=11.6865 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 08:06:24.51 +71:24:54.0: ref_mag=12.63 +/- 0.01 new_mean_mag=11.7113 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:29:38.86 +69:21:13.9: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:08:28.53 +68:28:28.5: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:29:38.86 +69:21:13.9: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 07:29:38.86 +69:21:13.9: ref_mag=12.68 +/- 0.01 new_mean_mag=11.5489 delta=1.13 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:34:41.64 +69:41:54.1: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:08:28.53 +68:28:28.5: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 07:08:28.53 +68:28:28.5: ref_mag=12.62 +/- 0.01 new_mean_mag=11.6686 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:34:41.64 +69:41:54.1: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 07:34:41.64 +69:41:54.1: ref_mag=12.57 +/- 0.01 new_mean_mag=11.6481 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:27:14.99 +69:29:51.9: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:27:14.99 +69:29:51.9: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 07:27:14.99 +69:29:51.9: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6535 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:59:03.24 +68:34:15.1: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:59:03.24 +68:34:15.1: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 06:59:03.24 +68:34:15.1: ref_mag=12.62 +/- 0.01 new_mean_mag=11.6819 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:51:30.71 +70:06:02.4: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:51:30.71 +70:06:02.4: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 07:51:30.71 +70:06:02.4: ref_mag=12.58 +/- 0.01 new_mean_mag=11.6763 delta=0.90 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:41:33.28 +70:58:55.4: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:41:33.28 +70:58:55.4: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 07:41:33.28 +70:58:55.4: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6644 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:18:01.45 +69:06:09.0: 12.59 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:18:01.45 +69:06:09.0: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 07:18:01.45 +69:06:09.0: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6503 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:09:02.18 +68:38:37.3: 12.59 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:09:02.18 +68:38:37.3: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:53:48.70 +68:17:09.0: 12.58 +/- 0.01 detection
Forced photometry filter KEPT candidate at 07:09:02.18 +68:38:37.3: ref_mag=12.60 +/- 0.01 new_mean_mag=11.6190 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:33:57.63 +69:22:08.1: 12.59 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:53:48.70 +68:17:09.0: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 06:53:48.70 +68:17:09.0: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6747 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:33:57.63 +69:22:08.1: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 07:33:57.63 +69:22:08.1: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6531 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 06:58:34.80 +68:01:58.6: 12.58 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 06:58:34.80 +68:01:58.6: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 06:58:34.80 +68:01:58.6: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6759 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:05:20.19 +68:24:13.3: 12.58 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:05:20.19 +68:24:13.3: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 07:05:20.19 +68:24:13.3: ref_mag=12.58 +/- 0.01 new_mean_mag=11.5800 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:46:21.87 +70:12:43.5: 12.57 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:46:21.87 +70:12:43.5: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 07:46:21.87 +70:12:43.5: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6398 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:07:17.32 +68:33:42.2: 12.56 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:07:17.32 +68:33:42.2: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 07:07:17.32 +68:33:42.2: ref_mag=12.57 +/- 0.01 new_mean_mag=11.6083 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:44:46.41 +70:58:43.7: 12.55 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:44:46.41 +70:58:43.7: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 07:44:46.41 +70:58:43.7: ref_mag=12.57 +/- 0.01 new_mean_mag=11.6152 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:35:13.42 +69:25:02.4: 12.54 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:35:13.42 +69:25:02.4: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 07:35:13.42 +69:25:02.4: ref_mag=12.54 +/- 0.01 new_mean_mag=11.6296 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:28:29.01 +69:38:20.1: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:28:29.01 +69:38:20.1: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 07:28:29.01 +69:38:20.1: ref_mag=12.55 +/- 0.01 new_mean_mag=11.5848 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:26:07.47 +70:11:17.3: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:26:07.47 +70:11:17.3: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 07:26:07.47 +70:11:17.3: ref_mag=12.54 +/- 0.01 new_mean_mag=11.5777 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:22:59.98 +69:52:43.9: 12.43 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:22:59.98 +69:52:43.9: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter KEPT candidate at 07:22:59.98 +69:52:43.9: ref_mag=12.41 +/- 0.01 new_mean_mag=11.4696 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:29:08.52 +70:26:35.0: 12.40 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:19:59.13 +69:33:17.0: 12.36 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:19:59.13 +69:33:17.0: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 07:19:59.13 +69:33:17.0: ref_mag=12.38 +/- 0.01 new_mean_mag=11.4178 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:29:08.52 +70:26:35.0: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter KEPT candidate at 07:29:08.52 +70:26:35.0: ref_mag=12.40 +/- 0.01 new_mean_mag=11.4498 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-07-Q2b1x1_2026-01-18_00-58-14_20.00sec_-15.00C_LIGHT_0286.fits at 07:29:04.65 +69:54:00.8: 12.32 +/- 0.01 detection
Forced photometry on wcs_Cam-07-Q2b1x1_2026-02-11_01-06-01_20.00sec_-15.00C_LIGHT_0290.fits at 07:29:04.65 +69:54:00.8: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 07:29:04.65 +69:54:00.8: ref_mag=12.34 +/- 0.01 new_mean_mag=11.4069 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out20002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46874.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out47192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82594.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 193s
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: 85s
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Considering the candidate 97075_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
The candidate 97075_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307 did not pass the final checks
**** FOUND 07:15:11.88 +68:48:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06621_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
The candidate 06621_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307 did not pass the final checks
**** FOUND 08:03:59.54 +73:24:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81633_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 81633_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 76157_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 76157_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 69162_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 69162_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46784_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46784_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41872_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41872_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40847_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 40847_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47613_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 47613_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82252_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 82252_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44359_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 44359_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36385_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 36385_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81977_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 81977_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56662_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 56662_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60240_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 60240_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39508_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 39508_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43553_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 43553_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38752_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 38752_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34779_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 34779_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58633_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 58633_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38552_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 38552_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59853_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 59853_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41545_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41545_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59526_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 59526_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39457_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 39457_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35696_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 35696_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46874_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46874_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40851_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 40851_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32960_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 32960_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61367_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 61367_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35700_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 35700_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47620_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 47620_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60920_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 60920_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46946_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46946_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45928_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 45928_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81742_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 81742_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33333_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 33333_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43679_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 43679_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76694_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 76694_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37394_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 37394_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81360_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 81360_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43634_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 43634_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77469_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 77469_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23817_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 23817_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35488_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 35488_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44300_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 44300_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82363_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 82363_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41005_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41005_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39830_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 39830_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77295_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 77295_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58832_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 58832_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35638_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 35638_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46243_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46243_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34155_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 34155_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82155_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 82155_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43064_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 43064_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78623_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 78623_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47807_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 47807_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45489_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 45489_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34632_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 34632_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47524_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 47524_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29090_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 29090_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60129_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 60129_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26854_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 26854_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44976_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 44976_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76730_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 76730_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45254_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 45254_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42543_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 42543_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76349_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 76349_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34579_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 34579_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35299_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 35299_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82436_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 82436_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25866_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 25866_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40603_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 40603_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41042_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41042_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60628_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 60628_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40007_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 40007_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82267_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 82267_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39004_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 39004_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 47192_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 47192_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 27625_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 27625_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 41211_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41211_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 80692_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 80692_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 60037_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 60037_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 38300_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 38300_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 44353_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 44353_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 81790_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 81790_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 40101_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 40101_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 47662_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 47662_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 37877_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 37877_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 46476_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46476_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 39686_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 39686_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 23005_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 23005_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 30426_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
The candidate 30426_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307 did not pass the final checks
**** FOUND 07:37:01.54 +70:45:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41845_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41845_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 46868_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46868_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 40760_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 40760_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 27597_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 27597_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 58252_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 58252_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 38930_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 38930_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 81714_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 81714_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 42909_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 42909_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 46655_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46655_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28373_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 28373_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 28933_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 28933_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 75558_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 75558_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26979_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 26979_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60852_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 60852_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37494_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 37494_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 29902_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 29902_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 30335_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 30335_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48388_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 48388_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41870_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41870_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25717_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 25717_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29301_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 29301_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 41689_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41689_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 82197_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 82197_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36898_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 36898_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38924_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 38924_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 31511_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 31511_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68386_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 68386_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34609_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 34609_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25225_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 25225_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58826_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 58826_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 78523_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 78523_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37972_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 37972_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57349_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 57349_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61350_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 61350_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46438_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46438_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36914_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 36914_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46704_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46704_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41725_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41725_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30770_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 30770_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32272_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 32272_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 32281_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 32281_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60850_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 60850_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20002_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 20002_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42647_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 42647_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82110_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 82110_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39162_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 39162_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41946_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41946_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82075_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 82075_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32866_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 32866_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27951_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 27951_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46395_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 46395_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58942_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 58942_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79897_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 79897_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41949_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41949_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78335_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 78335_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81355_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 81355_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33106_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 33106_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82594_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 82594_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 27527_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 27527_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 41285_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 41285_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
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Considering the candidate 40586_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 40586_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36554_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 36554_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58724_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
The candidate 58724_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307 did not pass the final checks
**** FOUND 07:14:51.58 +68:33:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39401_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 39401_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27876_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
The candidate 27876_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307 did not pass the final checks
**** FOUND 07:46:04.44 +70:53:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34040_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 34040_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42451_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 42451_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38401_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
Preparing report for the candidate 38401_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 287s
Prepared the HTML report for the field Cam-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:06:24.51 +71:24:54.0
08:01:22.23 +71:09:08.3
08:00:48.29 +71:04:00.7
07:49:43.74 +71:09:47.2
07:52:25.44 +71:01:40.1
07:54:58.91 +70:56:17.9
07:55:42.65 +70:47:35.4
07:47:20.20 +70:59:07.8
07:44:46.41 +70:58:43.7
07:49:58.51 +70:50:27.8
07:51:14.18 +70:48:26.0
07:41:33.28 +70:58:55.4
07:40:20.28 +70:57:34.0
07:45:09.50 +70:46:39.3
07:56:32.17 +70:28:04.7
07:46:31.52 +70:42:00.2
07:40:32.80 +70:45:07.3
07:37:23.16 +70:46:07.2
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07:43:22.88 +70:28:54.4
07:52:15.54 +70:09:55.5
07:53:34.49 +70:07:40.2
07:51:30.71 +70:06:02.4
07:51:40.73 +70:05:38.0
07:46:21.87 +70:12:43.5
07:45:01.61 +70:12:41.6
07:29:08.52 +70:26:35.0
07:42:51.67 +70:09:15.2
07:44:52.41 +70:02:49.3
07:32:12.40 +70:18:03.1
07:38:07.17 +70:11:47.8
07:27:43.80 +70:22:54.8
07:28:29.01 +70:17:57.9
07:33:09.72 +70:11:16.3
07:37:20.61 +70:05:24.9
07:28:25.71 +70:15:29.3
07:31:52.23 +70:11:36.1
07:42:38.33 +69:52:50.6
07:26:07.47 +70:11:17.3
07:29:49.08 +70:04:42.8
07:30:11.12 +70:04:13.8
07:38:46.17 +69:50:37.7
07:37:45.49 +69:50:39.7
07:31:15.47 +69:55:49.9
07:33:34.86 +69:52:19.8
07:25:33.65 +69:58:40.8
07:29:04.65 +69:54:00.8
07:26:36.83 +69:55:51.2
07:25:24.69 +69:55:46.4
07:21:27.01 +69:57:52.4
07:20:15.80 +69:59:00.0
07:31:13.74 +69:47:28.7
07:34:41.64 +69:41:54.1
07:22:59.98 +69:52:43.9
07:42:02.95 +69:30:29.5
07:31:17.48 +69:44:00.9
07:17:56.25 +69:55:49.4
07:21:12.26 +69:51:47.7
07:32:33.46 +69:38:25.7
07:24:11.97 +69:46:46.7
07:28:29.01 +69:38:20.1
07:38:36.42 +69:26:06.2
07:26:57.92 +69:38:46.3
07:22:13.49 +69:43:12.2
07:23:31.53 +69:41:38.4
07:26:53.20 +69:36:59.2
07:16:56.86 +69:45:49.6
07:16:21.43 +69:45:23.2
07:35:13.42 +69:25:02.4
07:20:20.58 +69:39:57.1
07:26:35.58 +69:32:09.5
07:25:14.18 +69:32:35.2
07:20:12.63 +69:37:34.0
07:14:43.77 +69:41:59.0
07:36:53.59 +69:19:06.4
07:27:14.99 +69:29:51.9
07:33:57.63 +69:22:08.1
07:19:59.13 +69:33:17.0
07:24:38.85 +69:28:29.8
07:29:38.86 +69:21:13.9
07:28:36.82 +69:21:04.4
07:32:47.31 +69:15:22.5
07:18:16.63 +69:27:16.0
07:32:24.75 +69:11:44.5
07:27:13.18 +69:16:24.3
07:20:35.25 +69:19:32.2
07:18:17.71 +69:21:20.7
07:27:10.47 +69:12:45.4
07:24:46.09 +69:10:48.8
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07:15:16.49 +69:15:43.0
07:12:37.64 +69:14:20.2
07:15:00.85 +69:10:10.3
07:18:01.45 +69:06:09.0
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07:18:28.44 +69:01:46.0
07:13:12.26 +69:06:50.9
07:10:34.32 +69:08:33.3
07:15:24.28 +69:02:49.3
07:24:31.04 +68:52:04.5
07:12:16.39 +69:02:11.2
07:10:49.16 +69:03:26.9
07:21:13.88 +68:54:04.7
07:19:31.74 +68:54:38.3
07:21:02.82 +68:48:47.0
06:56:17.55 +67:04:48.4
06:59:24.27 +67:41:53.4
07:00:56.07 +68:31:01.3
07:19:03.99 +68:28:18.0
07:04:46.76 +68:40:48.6
07:18:04.47 +68:30:24.4
07:09:02.18 +68:38:37.3
07:12:56.85 +68:41:01.4
07:12:31.55 +68:43:37.1
07:03:20.79 +68:51:23.6
07:02:59.89 +68:51:41.8
07:10:50.86 +68:48:23.3
07:12:04.83 +68:49:23.9
07:09:51.96 +68:53:48.7
07:11:14.70 +68:52:52.7
07:19:05.29 +68:47:59.5
07:14:29.80 +68:53:54.7
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06:32:38.27 +66:44:05.4
06:35:30.37 +66:49:57.7
07:01:39.70 +67:34:55.6
06:49:38.45 +67:46:49.0
06:47:54.29 +67:49:00.1
06:50:22.94 +67:50:41.8
06:51:23.11 +67:50:46.2
07:01:32.57 +67:50:03.9
07:05:22.33 +67:49:29.6
06:58:34.80 +68:01:58.6
06:56:02.82 +68:03:33.8
07:06:36.77 +67:58:40.6
06:53:48.70 +68:17:09.0
07:07:09.56 +68:17:39.4
07:05:20.19 +68:24:13.3
07:05:14.38 +68:24:21.4
06:59:43.71 +68:29:44.9
06:59:18.89 +68:30:40.6
07:05:36.84 +68:27:36.5
07:08:54.07 +68:27:37.8
07:08:40.22 +68:28:15.2
06:59:03.24 +68:34:15.1
07:08:28.53 +68:28:28.5
07:01:19.99 +68:34:29.6
07:00:26.92 +68:35:07.0
07:16:59.37 +68:23:57.3
07:03:55.84 +68:32:36.8
07:00:49.76 +68:35:40.3
06:58:11.14 +68:38:04.2
07:07:17.32 +68:33:42.2
Source monitoring: measuring positions from /data_ssd/NMW-TexasTech/workdir/img_2026-08-06_CI_Cam-07-Q2b1x1_024122_TTUQ2b1x1_4009071_kZUuYvoM/monitoring_positions.txt
Read 9788 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 79.6591 to 135.4309 deg, Dec +63.2921 to +75.2508 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 79.6591 to 135.4309 deg, Dec 63.2921 to 75.2508 deg
Loaded 12263 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): 5931 out of 6057 total matches.
Matched with Tycho-2 6057 out of 9788 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits
Observation time (mid-exposure, UTC): JD 2461258.80535 (FITS header)
Observing site: lat= +33.748292 deg lon= -101.958319 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 108.02977 deg Dec= +69.96901 deg
Frame center: alt= +16.740 deg az= 14.073 deg airmass= 3.4232
Header cross-check: CENTALT= 16.618 deg (difference +0.122 deg)
Header cross-check: AIRMASS= 3.4579 (we compute 3.4232)
Airmass zero-point fit: REJECT_K_RANGE k= -0.3822 +/- 0.0105 mag/airmass N= 4410 airmass span 2.3919-5.8947 scatter 0.4753 mag
Source monitoring: airmass zero-point for wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits: REJECT_K_RANGE -1.412755 +0.382214 3.4232 -0.3822 4410 3.5028 0.4753 2.3919 5.8947
Forced photometry (list mode): image=wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits list=monitoring_pixlist4010835.tmp aperture=4.4
Image size: 9576 x 6388
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 20.439900
Forced photometry: center=(5315.92, 4000.15) aperture=4.4
Annulus: inner=8.80 outer=22.00
Background annulus: 1275 pixels
Iterative clipping converged after 3 iterations, 1268/1275 pixels remain
SExtractor background: mode=1999.26 median=1999.50 mean=1999.66 sigma=65.55 -> bg=1999.26 (1268 pixels)
Aperture sum=30473.90 N_eff=15.2053
Net flux=74.58 noise=255.61 SNR=0.29
Instrumental magnitude: -7.2117
Calibrated magnitude: 13.2282
Source monitoring: 1 position(s) measured on wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-19-31_20.00sec_-0.00C_LIGHT_0306.fits (aperture 4.4 pix)
Read 10063 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 79.6613 to 135.4306 deg, Dec +63.2925 to +75.2856 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 79.6613 to 135.4306 deg, Dec 63.2925 to 75.2856 deg
Loaded 12288 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): 6032 out of 6154 total matches.
Matched with Tycho-2 6154 out of 10063 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits
Observation time (mid-exposure, UTC): JD 2461258.80597 (FITS header)
Observing site: lat= +33.748292 deg lon= -101.958319 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 108.03657 deg Dec= +69.97811 deg
Frame center: alt= +16.784 deg az= 14.147 deg airmass= 3.4146
Header cross-check: CENTALT= 16.656 deg (difference +0.129 deg)
Header cross-check: AIRMASS= 3.4504 (we compute 3.4146)
Airmass zero-point fit: REJECT_K_RANGE k= -0.3548 +/- 0.0105 mag/airmass N= 4508 airmass span 2.3815-5.8797 scatter 0.4768 mag
Source monitoring: airmass zero-point for wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits: REJECT_K_RANGE -1.313440 +0.354805 3.4146 -0.3548 4508 3.4982 0.4768 2.3815 5.8797
Forced photometry (list mode): image=wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits list=monitoring_pixlist4010835.tmp aperture=4.4
Image size: 9576 x 6388
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 20.477750
Forced photometry: center=(5314.19, 3994.74) aperture=4.4
Annulus: inner=8.80 outer=22.00
Background annulus: 1282 pixels
Iterative clipping converged after 3 iterations, 1273/1282 pixels remain
SExtractor background: mode=1947.98 median=1949.00 mean=1949.68 sigma=62.90 -> bg=1947.98 (1273 pixels)
Aperture sum=29754.44 N_eff=15.2053
Net flux=134.79 noise=245.26 SNR=0.55
Instrumental magnitude: -7.1669
Calibrated magnitude: 13.3109
Source monitoring: 1 position(s) measured on wcs_fd_Cam-07-Q2b1x1_2026-08-06_02-20-25_20.00sec_-0.00C_LIGHT_0307.fits (aperture 4.4 pix)
########### Completed Cam-07-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:59:43.71 +68:29:44.9
06:49:38.45 +67:46:49.0
06:35:30.37 +66:49:57.7
07:13:53.42 +69:06:52.7
07:36:53.59 +69:19:06.4
07:22:13.49 +69:43:12.2
07:12:16.39 +69:02:11.2
07:16:59.37 +68:23:57.3
07:27:10.47 +69:12:45.4
07:42:38.33 +69:52:50.6
07:08:40.22 +68:28:15.2
06:56:17.55 +67:04:48.4
07:10:50.86 +68:48:23.3
07:31:17.48 +69:44:00.9
07:18:16.63 +69:27:16.0
07:25:24.69 +69:55:46.4
07:27:43.80 +70:22:54.8
07:19:03.99 +68:28:18.0
07:26:36.83 +69:55:51.2
07:12:31.55 +68:43:37.1
07:20:20.58 +69:39:57.1
07:12:56.85 +68:41:01.4
07:42:02.95 +69:30:29.5
07:28:25.71 +70:15:29.3
07:13:12.26 +69:06:50.9
07:23:31.53 +69:41:38.4
07:51:40.73 +70:05:38.0
07:14:16.22 +68:53:47.3
07:31:52.23 +70:11:36.1
07:10:49.16 +69:03:26.9
07:19:05.29 +68:47:59.5
07:10:34.32 +69:08:33.3
07:12:37.64 +69:14:20.2
07:05:36.84 +68:27:36.5
07:45:01.61 +70:12:41.6
07:27:13.18 +69:16:24.3
06:50:22.94 +67:50:41.8
07:38:46.17 +69:50:37.7
07:05:14.38 +68:24:21.4
07:32:24.75 +69:11:44.5
07:05:22.33 +67:49:29.6
08:00:48.29 +71:04:00.7
07:33:09.72 +70:11:16.3
07:20:35.25 +69:19:32.2
07:00:49.76 +68:35:40.3
07:26:53.20 +69:36:59.2
07:21:12.26 +69:51:47.7
07:01:32.57 +67:50:03.9
07:18:04.47 +68:30:24.4
07:37:20.61 +70:05:24.9
07:15:00.85 +69:10:10.3
07:42:51.67 +70:09:15.2
07:01:19.99 +68:34:29.6
07:32:47.31 +69:15:22.5
07:06:36.77 +67:58:40.6
07:19:31.74 +68:54:38.3
07:15:16.49 +69:15:43.0
07:38:07.17 +70:11:47.8
07:24:31.04 +68:52:04.5
07:56:32.17 +70:28:04.7
07:02:59.89 +68:51:41.8
07:55:42.65 +70:47:35.4
07:24:46.09 +69:10:48.8
06:51:23.11 +67:50:46.2
07:23:42.13 +69:09:33.0
07:24:38.85 +69:28:29.8
06:47:54.29 +67:49:00.1
07:44:52.41 +70:02:49.3
07:28:29.01 +70:17:57.9
06:58:11.14 +68:38:04.2
07:54:58.91 +70:56:17.9
07:38:36.42 +69:26:06.2
07:16:56.86 +69:45:49.6
07:12:04.83 +68:49:23.9
07:32:33.46 +69:38:25.7
07:03:55.84 +68:32:36.8
07:31:13.74 +69:47:28.7
07:15:24.28 +69:02:49.3
07:51:14.18 +70:48:26.0
07:16:21.43 +69:45:23.2
07:07:09.56 +68:17:39.4
07:03:20.79 +68:51:23.6
07:25:33.65 +69:58:40.8
07:18:17.71 +69:21:20.7
07:08:54.07 +68:27:37.8
07:24:11.97 +69:46:46.7
07:21:13.88 +68:54:04.7
07:31:15.47 +69:55:49.9
07:20:06.48 +69:03:59.2
07:17:56.25 +69:55:49.4
08:01:22.23 +71:09:08.3
07:20:12.63 +69:37:34.0
07:18:28.44 +69:01:46.0
07:26:57.92 +69:38:46.3
07:49:58.51 +70:50:27.8
07:00:56.07 +68:31:01.3
07:20:15.80 +69:59:00.0
06:59:18.89 +68:30:40.6
07:28:36.82 +69:21:04.4
07:12:56.85 +69:08:25.5
07:40:20.28 +70:57:34.0
07:45:09.50 +70:46:39.3
07:01:39.70 +67:34:55.6
07:47:20.20 +70:59:07.8
07:11:14.70 +68:52:52.7
07:37:45.49 +69:50:39.7
07:40:32.80 +70:45:07.3
07:37:23.16 +70:46:07.2
07:21:02.82 +68:48:47.0
07:14:43.77 +69:41:59.0
07:52:25.44 +71:01:40.1
07:46:31.52 +70:42:00.2
07:26:35.58 +69:32:09.5
07:00:26.92 +68:35:07.0
07:29:49.08 +70:04:42.8
07:21:27.01 +69:57:52.4
07:43:22.88 +70:28:54.4
06:32:38.27 +66:44:05.4
07:32:12.40 +70:18:03.1
07:49:43.74 +71:09:47.2
07:04:46.76 +68:40:48.6
06:56:02.82 +68:03:33.8
07:33:34.86 +69:52:19.8
06:59:24.27 +67:41:53.4
07:14:29.80 +68:53:54.7
07:13:08.88 +69:09:51.7
07:30:11.12 +70:04:13.8
07:21:11.04 +69:01:00.5
07:25:14.18 +69:32:35.2
07:47:18.35 +70:29:00.4
07:52:15.54 +70:09:55.5
07:53:34.49 +70:07:40.2
07:09:51.96 +68:53:48.7
08:06:24.51 +71:24:54.0
07:29:38.86 +69:21:13.9
07:08:28.53 +68:28:28.5
07:34:41.64 +69:41:54.1
07:27:14.99 +69:29:51.9
06:59:03.24 +68:34:15.1
07:51:30.71 +70:06:02.4
07:41:33.28 +70:58:55.4
07:18:01.45 +69:06:09.0
07:09:02.18 +68:38:37.3
06:53:48.70 +68:17:09.0
07:33:57.63 +69:22:08.1
06:58:34.80 +68:01:58.6
07:05:20.19 +68:24:13.3
07:46:21.87 +70:12:43.5
07:07:17.32 +68:33:42.2
07:44:46.41 +70:58:43.7
07:35:13.42 +69:25:02.4
07:28:29.01 +69:38:20.1
07:26:07.47 +70:11:17.3
07:22:59.98 +69:52:43.9
07:29:08.52 +70:26:35.0
07:19:59.13 +69:33:17.0
07:29:04.65 +69:54:00.8
###################################################################################
06:59:43.71 +68:29:44.9 -- not an asteroid (will add it to exclusion list)
06:49:38.45 +67:46:49.0 -- not an asteroid (will add it to exclusion list)
06:35:30.37 +66:49:57.7 -- not an asteroid (will add it to exclusion list)
07:13:53.42 +69:06:52.7 -- not an asteroid (will add it to exclusion list)
07:36:53.59 +69:19:06.4 -- not an asteroid (will add it to exclusion list)
07:22:13.49 +69:43:12.2 -- not an asteroid (will add it to exclusion list)
07:12:16.39 +69:02:11.2 -- not an asteroid (will add it to exclusion list)
07:16:59.37 +68:23:57.3 -- not an asteroid (will add it to exclusion list)
07:27:10.47 +69:12:45.4 -- not an asteroid (will add it to exclusion list)
07:42:38.33 +69:52:50.6 -- not an asteroid (will add it to exclusion list)
07:08:40.22 +68:28:15.2 -- not an asteroid (will add it to exclusion list)
06:56:17.55 +67:04:48.4 -- not an asteroid (will add it to exclusion list)
07:10:50.86 +68:48:23.3 -- not an asteroid (will add it to exclusion list)
07:31:17.48 +69:44:00.9 -- not an asteroid (will add it to exclusion list)
07:18:16.63 +69:27:16.0 -- not an asteroid (will add it to exclusion list)
07:25:24.69 +69:55:46.4 -- not an asteroid (will add it to exclusion list)
07:27:43.80 +70:22:54.8 -- not an asteroid (will add it to exclusion list)
07:19:03.99 +68:28:18.0 -- not an asteroid (will add it to exclusion list)
07:26:36.83 +69:55:51.2 -- not an asteroid (will add it to exclusion list)
07:12:31.55 +68:43:37.1 -- not an asteroid (will add it to exclusion list)
07:20:20.58 +69:39:57.1 -- not an asteroid (will add it to exclusion list)
07:12:56.85 +68:41:01.4 -- not an asteroid (will add it to exclusion list)
07:42:02.95 +69:30:29.5 -- not an asteroid (will add it to exclusion list)
07:28:25.71 +70:15:29.3 -- not an asteroid (will add it to exclusion list)
07:13:12.26 +69:06:50.9 -- not an asteroid (will add it to exclusion list)
07:23:31.53 +69:41:38.4 -- not an asteroid (will add it to exclusion list)
07:51:40.73 +70:05:38.0 -- not an asteroid (will add it to exclusion list)
07:14:16.22 +68:53:47.3 -- not an asteroid (will add it to exclusion list)
07:31:52.23 +70:11:36.1 -- not an asteroid (will add it to exclusion list)
07:10:49.16 +69:03:26.9 -- not an asteroid (will add it to exclusion list)
07:19:05.29 +68:47:59.5 -- not an asteroid (will add it to exclusion list)
07:10:34.32 +69:08:33.3 -- not an asteroid (will add it to exclusion list)
07:12:37.64 +69:14:20.2 -- not an asteroid (will add it to exclusion list)
07:05:36.84 +68:27:36.5 -- not an asteroid (will add it to exclusion list)
07:45:01.61 +70:12:41.6 -- not an asteroid (will add it to exclusion list)
07:27:13.18 +69:16:24.3 -- not an asteroid (will add it to exclusion list)
06:50:22.94 +67:50:41.8 -- not an asteroid (will add it to exclusion list)
07:38:46.17 +69:50:37.7 -- not an asteroid (will add it to exclusion list)
07:05:14.38 +68:24:21.4 -- not an asteroid (will add it to exclusion list)
07:32:24.75 +69:11:44.5 -- not an asteroid (will add it to exclusion list)
07:05:22.33 +67:49:29.6 -- not an asteroid (will add it to exclusion list)
08:00:48.29 +71:04:00.7 -- not an asteroid (will add it to exclusion list)
07:33:09.72 +70:11:16.3 -- not an asteroid (will add it to exclusion list)
07:20:35.25 +69:19:32.2 -- not an asteroid (will add it to exclusion list)
07:00:49.76 +68:35:40.3 -- not an asteroid (will add it to exclusion list)
07:26:53.20 +69:36:59.2 -- not an asteroid (will add it to exclusion list)
07:21:12.26 +69:51:47.7 -- not an asteroid (will add it to exclusion list)
07:01:32.57 +67:50:03.9 -- not an asteroid (will add it to exclusion list)
07:18:04.47 +68:30:24.4 -- not an asteroid (will add it to exclusion list)
07:37:20.61 +70:05:24.9 -- not an asteroid (will add it to exclusion list)
07:15:00.85 +69:10:10.3 -- not an asteroid (will add it to exclusion list)
07:42:51.67 +70:09:15.2 -- not an asteroid (will add it to exclusion list)
07:01:19.99 +68:34:29.6 -- not an asteroid (will add it to exclusion list)
07:32:47.31 +69:15:22.5 -- not an asteroid (will add it to exclusion list)
07:06:36.77 +67:58:40.6 -- not an asteroid (will add it to exclusion list)
07:19:31.74 +68:54:38.3 -- not an asteroid (will add it to exclusion list)
07:15:16.49 +69:15:43.0 -- not an asteroid (will add it to exclusion list)
07:38:07.17 +70:11:47.8 -- not an asteroid (will add it to exclusion list)
07:24:31.04 +68:52:04.5 -- not an asteroid (will add it to exclusion list)
07:56:32.17 +70:28:04.7 -- not an asteroid (will add it to exclusion list)
07:02:59.89 +68:51:41.8 -- not an asteroid (will add it to exclusion list)
07:55:42.65 +70:47:35.4 -- not an asteroid (will add it to exclusion list)
07:24:46.09 +69:10:48.8 -- not an asteroid (will add it to exclusion list)
06:51:23.11 +67:50:46.2 -- not an asteroid (will add it to exclusion list)
07:23:42.13 +69:09:33.0 -- not an asteroid (will add it to exclusion list)
07:24:38.85 +69:28:29.8 -- not an asteroid (will add it to exclusion list)
06:47:54.29 +67:49:00.1 -- not an asteroid (will add it to exclusion list)
07:44:52.41 +70:02:49.3 -- not an asteroid (will add it to exclusion list)
07:28:29.01 +70:17:57.9 -- not an asteroid (will add it to exclusion list)
06:58:11.14 +68:38:04.2 -- not an asteroid (will add it to exclusion list)
07:54:58.91 +70:56:17.9 -- not an asteroid (will add it to exclusion list)
07:38:36.42 +69:26:06.2 -- not an asteroid (will add it to exclusion list)
07:16:56.86 +69:45:49.6 -- not an asteroid (will add it to exclusion list)
07:12:04.83 +68:49:23.9 -- not an asteroid (will add it to exclusion list)
07:32:33.46 +69:38:25.7 -- not an asteroid (will add it to exclusion list)
07:03:55.84 +68:32:36.8 -- not an asteroid (will add it to exclusion list)
07:31:13.74 +69:47:28.7 -- not an asteroid (will add it to exclusion list)
07:15:24.28 +69:02:49.3 -- not an asteroid (will add it to exclusion list)
07:51:14.18 +70:48:26.0 -- not an asteroid (will add it to exclusion list)
07:16:21.43 +69:45:23.2 -- not an asteroid (will add it to exclusion list)
07:07:09.56 +68:17:39.4 -- not an asteroid (will add it to exclusion list)
07:03:20.79 +68:51:23.6 -- not an asteroid (will add it to exclusion list)
07:25:33.65 +69:58:40.8 -- not an asteroid (will add it to exclusion list)
07:18:17.71 +69:21:20.7 -- not an asteroid (will add it to exclusion list)
07:08:54.07 +68:27:37.8 -- not an asteroid (will add it to exclusion list)
07:24:11.97 +69:46:46.7 -- not an asteroid (will add it to exclusion list)
07:21:13.88 +68:54:04.7 -- not an asteroid (will add it to exclusion list)
07:31:15.47 +69:55:49.9 -- not an asteroid (will add it to exclusion list)
07:20:06.48 +69:03:59.2 -- not an asteroid (will add it to exclusion list)
07:17:56.25 +69:55:49.4 -- not an asteroid (will add it to exclusion list)
08:01:22.23 +71:09:08.3 -- not an asteroid (will add it to exclusion list)
07:20:12.63 +69:37:34.0 -- not an asteroid (will add it to exclusion list)
07:18:28.44 +69:01:46.0 -- not an asteroid (will add it to exclusion list)
07:26:57.92 +69:38:46.3 -- not an asteroid (will add it to exclusion list)
07:49:58.51 +70:50:27.8 -- not an asteroid (will add it to exclusion list)
07:00:56.07 +68:31:01.3 -- not an asteroid (will add it to exclusion list)
07:20:15.80 +69:59:00.0 -- not an asteroid (will add it to exclusion list)
06:59:18.89 +68:30:40.6 -- not an asteroid (will add it to exclusion list)
07:28:36.82 +69:21:04.4 -- not an asteroid (will add it to exclusion list)
07:12:56.85 +69:08:25.5 -- not an asteroid (will add it to exclusion list)
07:40:20.28 +70:57:34.0 -- not an asteroid (will add it to exclusion list)
07:45:09.50 +70:46:39.3 -- not an asteroid (will add it to exclusion list)
07:01:39.70 +67:34:55.6 -- not an asteroid (will add it to exclusion list)
07:47:20.20 +70:59:07.8 -- not an asteroid (will add it to exclusion list)
07:11:14.70 +68:52:52.7 -- not an asteroid (will add it to exclusion list)
07:37:45.49 +69:50:39.7 -- not an asteroid (will add it to exclusion list)
07:40:32.80 +70:45:07.3 -- not an asteroid (will add it to exclusion list)
07:37:23.16 +70:46:07.2 -- not an asteroid (will add it to exclusion list)
07:21:02.82 +68:48:47.0 -- not an asteroid (will add it to exclusion list)
07:14:43.77 +69:41:59.0 -- not an asteroid (will add it to exclusion list)
07:52:25.44 +71:01:40.1 -- not an asteroid (will add it to exclusion list)
07:46:31.52 +70:42:00.2 -- not an asteroid (will add it to exclusion list)
07:26:35.58 +69:32:09.5 -- not an asteroid (will add it to exclusion list)
07:00:26.92 +68:35:07.0 -- not an asteroid (will add it to exclusion list)
07:29:49.08 +70:04:42.8 -- not an asteroid (will add it to exclusion list)
07:21:27.01 +69:57:52.4 -- not an asteroid (will add it to exclusion list)
07:43:22.88 +70:28:54.4 -- not an asteroid (will add it to exclusion list)
06:32:38.27 +66:44:05.4 -- not an asteroid (will add it to exclusion list)
07:32:12.40 +70:18:03.1 -- not an asteroid (will add it to exclusion list)
07:49:43.74 +71:09:47.2 -- not an asteroid (will add it to exclusion list)
07:04:46.76 +68:40:48.6 -- not an asteroid (will add it to exclusion list)
06:56:02.82 +68:03:33.8 -- not an asteroid (will add it to exclusion list)
07:33:34.86 +69:52:19.8 -- not an asteroid (will add it to exclusion list)
06:59:24.27 +67:41:53.4 -- not an asteroid (will add it to exclusion list)
07:14:29.80 +68:53:54.7 -- not an asteroid (will add it to exclusion list)
07:13:08.88 +69:09:51.7 -- not an asteroid (will add it to exclusion list)
07:30:11.12 +70:04:13.8 -- not an asteroid (will add it to exclusion list)
07:21:11.04 +69:01:00.5 -- not an asteroid (will add it to exclusion list)
07:25:14.18 +69:32:35.2 -- not an asteroid (will add it to exclusion list)
07:47:18.35 +70:29:00.4 -- not an asteroid (will add it to exclusion list)
07:52:15.54 +70:09:55.5 -- not an asteroid (will add it to exclusion list)
07:53:34.49 +70:07:40.2 -- not an asteroid (will add it to exclusion list)
07:09:51.96 +68:53:48.7 -- not an asteroid (will add it to exclusion list)
08:06:24.51 +71:24:54.0 -- not an asteroid (will add it to exclusion list)
07:29:38.86 +69:21:13.9 -- not an asteroid (will add it to exclusion list)
07:08:28.53 +68:28:28.5 -- not an asteroid (will add it to exclusion list)
07:34:41.64 +69:41:54.1 -- not an asteroid (will add it to exclusion list)
07:27:14.99 +69:29:51.9 -- not an asteroid (will add it to exclusion list)
06:59:03.24 +68:34:15.1 -- not an asteroid (will add it to exclusion list)
07:51:30.71 +70:06:02.4 -- not an asteroid (will add it to exclusion list)
07:41:33.28 +70:58:55.4 -- not an asteroid (will add it to exclusion list)
07:18:01.45 +69:06:09.0 -- not an asteroid (will add it to exclusion list)
07:09:02.18 +68:38:37.3 -- not an asteroid (will add it to exclusion list)
06:53:48.70 +68:17:09.0 -- not an asteroid (will add it to exclusion list)
07:33:57.63 +69:22:08.1 -- not an asteroid (will add it to exclusion list)
06:58:34.80 +68:01:58.6 -- not an asteroid (will add it to exclusion list)
07:05:20.19 +68:24:13.3 -- not an asteroid (will add it to exclusion list)
07:46:21.87 +70:12:43.5 -- not an asteroid (will add it to exclusion list)
07:07:17.32 +68:33:42.2 -- not an asteroid (will add it to exclusion list)
07:44:46.41 +70:58:43.7 -- not an asteroid (will add it to exclusion list)
07:35:13.42 +69:25:02.4 -- not an asteroid (will add it to exclusion list)
07:28:29.01 +69:38:20.1 -- not an asteroid (will add it to exclusion list)
07:26:07.47 +70:11:17.3 -- not an asteroid (will add it to exclusion list)
07:22:59.98 +69:52:43.9 -- not an asteroid (will add it to exclusion list)
07:29:08.52 +70:26:35.0 -- not an asteroid (will add it to exclusion list)
07:19:59.13 +69:33:17.0 -- not an asteroid (will add it to exclusion list)
07:29:04.65 +69:54:00.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:32:38.27 +66:44:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:30.37 +66:49:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:54.29 +67:49:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:38.45 +67:46:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:22.94 +67:50:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:23.11 +67:50:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:48.70 +68:17:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:02.82 +68:03:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:17.55 +67:04:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:11.14 +68:38:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.80 +68:01:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:03.24 +68:34:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:18.89 +68:30:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:24.27 +67:41:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:43.71 +68:29:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:26.92 +68:35:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:49.76 +68:35:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:56.07 +68:31:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:19.99 +68:34:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:32.57 +67:50:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:39.70 +67:34:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:59.89 +68:51:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:20.79 +68:51:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:55.84 +68:32:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:46.76 +68:40:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:14.38 +68:24:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:20.19 +68:24:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:22.33 +67:49:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:36.84 +68:27:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:36.77 +67:58:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:09.56 +68:17:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:17.32 +68:33:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:28.53 +68:28:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:40.22 +68:28:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:54.07 +68:27:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:02.18 +68:38:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:51.96 +68:53:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:34.32 +69:08:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:49.16 +69:03:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:50.86 +68:48:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:14.70 +68:52:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:04.83 +68:49:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:16.39 +69:02:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:31.55 +68:43:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:37.64 +69:14:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:56.85 +68:41:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:56.85 +69:08:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:08.88 +69:09:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:12.26 +69:06:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:53.42 +69:06:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:16.22 +68:53:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:29.80 +68:53:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:43.77 +69:41:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:00.85 +69:10:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:16.49 +69:15:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:24.28 +69:02:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:21.43 +69:45:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:56.86 +69:45:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:59.37 +68:23:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:56.25 +69:55:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:01.45 +69:06:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:04.47 +68:30:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:16.63 +69:27:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:17.71 +69:21:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:28.44 +69:01:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:03.99 +68:28:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:05.29 +68:47:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:31.74 +68:54:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:59.13 +69:33:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:06.48 +69:03:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:12.63 +69:37:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:15.80 +69:59:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:20.58 +69:39:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:35.25 +69:19:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:02.82 +68:48:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:11.04 +69:01:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:12.26 +69:51:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:13.88 +68:54:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:27.01 +69:57:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:13.49 +69:43:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:59.98 +69:52:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:23:31.53 +69:41:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:23:42.13 +69:09:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:24:11.97 +69:46:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:24:31.04 +68:52:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:24:38.85 +69:28:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:24:46.09 +69:10:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:25:14.18 +69:32:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:25:24.69 +69:55:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:25:33.65 +69:58:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:26:07.47 +70:11:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:26:35.58 +69:32:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:26:36.83 +69:55:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:26:53.20 +69:36:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:26:57.92 +69:38:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:27:10.47 +69:12:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:27:13.18 +69:16:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:27:14.99 +69:29:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:27:43.80 +70:22:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:28:25.71 +70:15:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:28:29.01 +69:38:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:28:29.01 +70:17:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:28:36.82 +69:21:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:29:04.65 +69:54:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:29:08.52 +70:26:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:29:38.86 +69:21:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:29:49.08 +70:04:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:30:11.12 +70:04:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:31:13.74 +69:47:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:31:15.47 +69:55:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:31:17.48 +69:44:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:31:52.23 +70:11:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:32:12.40 +70:18:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:32:24.75 +69:11:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:32:33.46 +69:38:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:32:47.31 +69:15:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:33:09.72 +70:11:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:33:34.86 +69:52:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:33:57.63 +69:22:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:41.64 +69:41:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:13.42 +69:25:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:53.59 +69:19:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:20.61 +70:05:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:23.16 +70:46:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:45.49 +69:50:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:07.17 +70:11:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:36.42 +69:26:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:46.17 +69:50:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:20.28 +70:57:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:32.80 +70:45:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:33.28 +70:58:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:02.95 +69:30:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:38.33 +69:52:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:51.67 +70:09:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:22.88 +70:28:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:46.41 +70:58:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:52.41 +70:02:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:01.61 +70:12:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:09.50 +70:46:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:21.87 +70:12:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:31.52 +70:42:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:47:18.35 +70:29:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:47:20.20 +70:59:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:49:43.74 +71:09:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:49:58.51 +70:50:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:51:14.18 +70:48:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:51:30.71 +70:06:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:51:40.73 +70:05:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:52:15.54 +70:09:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:52:25.44 +71:01:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:53:34.49 +70:07:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:54:58.91 +70:56:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:55:42.65 +70:47:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:56:32.17 +70:28:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:00:48.29 +71:04:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:01:22.23 +71:09:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:06:24.51 +71:24:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:32:38.27 +66:44:05.4 -- not a known variable star
06:35:30.37 +66:49:57.7 -- not a known variable star
06:47:54.29 +67:49:00.1 -- not a known variable star
06:49:38.45 +67:46:49.0 -- not a known variable star
06:50:22.94 +67:50:41.8 -- not a known variable star
06:51:23.11 +67:50:46.2 -- not a known variable star
06:53:48.70 +68:17:09.0 -- not a known variable star
06:56:02.82 +68:03:33.8 -- not a known variable star
06:56:17.55 +67:04:48.4 -- a known variable star
06:58:11.14 +68:38:04.2 -- not a known variable star
06:58:34.80 +68:01:58.6 -- not a known variable star
06:59:03.24 +68:34:15.1 -- not a known variable star
06:59:18.89 +68:30:40.6 -- not a known variable star
06:59:24.27 +67:41:53.4 -- not a known variable star
06:59:43.71 +68:29:44.9 -- not a known variable star
07:00:26.92 +68:35:07.0 -- not a known variable star
07:00:49.76 +68:35:40.3 -- not a known variable star
07:00:56.07 +68:31:01.3 -- not a known variable star
07:01:19.99 +68:34:29.6 -- not a known variable star
07:01:32.57 +67:50:03.9 -- not a known variable star
07:01:39.70 +67:34:55.6 -- not a known variable star
07:02:59.89 +68:51:41.8 -- not a known variable star
07:03:20.79 +68:51:23.6 -- not a known variable star
07:03:55.84 +68:32:36.8 -- a known variable star
07:04:46.76 +68:40:48.6 -- not a known variable star
07:05:14.38 +68:24:21.4 -- a known variable star
07:05:20.19 +68:24:13.3 -- not a known variable star
07:05:22.33 +67:49:29.6 -- a known variable star
07:05:36.84 +68:27:36.5 -- not a known variable star
07:06:36.77 +67:58:40.6 -- a known variable star
07:07:09.56 +68:17:39.4 -- not a known variable star
07:07:17.32 +68:33:42.2 -- not a known variable star
07:08:28.53 +68:28:28.5 -- not a known variable star
07:08:40.22 +68:28:15.2 -- not a known variable star
07:08:54.07 +68:27:37.8 -- not a known variable star
07:09:02.18 +68:38:37.3 -- not a known variable star
07:09:51.96 +68:53:48.7 -- not a known variable star
07:10:34.32 +69:08:33.3 -- not a known variable star
07:10:49.16 +69:03:26.9 -- not a known variable star
07:10:50.86 +68:48:23.3 -- not a known variable star
07:11:14.70 +68:52:52.7 -- a known variable star
07:12:04.83 +68:49:23.9 -- not a known variable star
07:12:16.39 +69:02:11.2 -- not a known variable star
07:12:31.55 +68:43:37.1 -- a known variable star
07:12:37.64 +69:14:20.2 -- not a known variable star
07:12:56.85 +68:41:01.4 -- not a known variable star
07:12:56.85 +69:08:25.5 -- not a known variable star
07:13:08.88 +69:09:51.7 -- not a known variable star
07:13:12.26 +69:06:50.9 -- not a known variable star
07:13:53.42 +69:06:52.7 -- not a known variable star
07:14:16.22 +68:53:47.3 -- not a known variable star
07:14:29.80 +68:53:54.7 -- not a known variable star
07:14:43.77 +69:41:59.0 -- a known variable star
07:15:00.85 +69:10:10.3 -- not a known variable star
07:15:16.49 +69:15:43.0 -- not a known variable star
07:15:24.28 +69:02:49.3 -- not a known variable star
07:16:21.43 +69:45:23.2 -- not a known variable star
07:16:56.86 +69:45:49.6 -- not a known variable star
07:16:59.37 +68:23:57.3 -- not a known variable star
07:17:56.25 +69:55:49.4 -- not a known variable star
07:18:01.45 +69:06:09.0 -- not a known variable star
07:18:04.47 +68:30:24.4 -- not a known variable star
07:18:16.63 +69:27:16.0 -- not a known variable star
07:18:17.71 +69:21:20.7 -- not a known variable star
07:18:28.44 +69:01:46.0 -- not a known variable star
07:19:03.99 +68:28:18.0 -- a known variable star
07:19:05.29 +68:47:59.5 -- not a known variable star
07:19:31.74 +68:54:38.3 -- not a known variable star
07:19:59.13 +69:33:17.0 -- not a known variable star
07:20:06.48 +69:03:59.2 -- not a known variable star
07:20:12.63 +69:37:34.0 -- not a known variable star
07:20:15.80 +69:59:00.0 -- not a known variable star
07:20:20.58 +69:39:57.1 -- not a known variable star
07:20:35.25 +69:19:32.2 -- not a known variable star
07:21:02.82 +68:48:47.0 -- not a known variable star
07:21:11.04 +69:01:00.5 -- not a known variable star
07:21:12.26 +69:51:47.7 -- not a known variable star
07:21:13.88 +68:54:04.7 -- not a known variable star
07:21:27.01 +69:57:52.4 -- not a known variable star
07:22:13.49 +69:43:12.2 -- not a known variable star
07:22:59.98 +69:52:43.9 -- not a known variable star
07:23:31.53 +69:41:38.4 -- not a known variable star
07:23:42.13 +69:09:33.0 -- not a known variable star
07:24:11.97 +69:46:46.7 -- not a known variable star
07:24:31.04 +68:52:04.5 -- not a known variable star
07:24:38.85 +69:28:29.8 -- not a known variable star
07:24:46.09 +69:10:48.8 -- a known variable star
07:25:14.18 +69:32:35.2 -- not a known variable star
07:25:24.69 +69:55:46.4 -- a known variable star
07:25:33.65 +69:58:40.8 -- not a known variable star
07:26:07.47 +70:11:17.3 -- not a known variable star
07:26:35.58 +69:32:09.5 -- not a known variable star
07:26:36.83 +69:55:51.2 -- not a known variable star
07:26:53.20 +69:36:59.2 -- not a known variable star
07:26:57.92 +69:38:46.3 -- not a known variable star
07:27:10.47 +69:12:45.4 -- not a known variable star
07:27:13.18 +69:16:24.3 -- not a known variable star
07:27:14.99 +69:29:51.9 -- not a known variable star
07:27:43.80 +70:22:54.8 -- not a known variable star
07:28:25.71 +70:15:29.3 -- not a known variable star
07:28:29.01 +69:38:20.1 -- not a known variable star
07:28:29.01 +70:17:57.9 -- a known variable star
07:28:36.82 +69:21:04.4 -- not a known variable star
07:29:04.65 +69:54:00.8 -- not a known variable star
07:29:08.52 +70:26:35.0 -- not a known variable star
07:29:38.86 +69:21:13.9 -- a known variable star
07:29:49.08 +70:04:42.8 -- not a known variable star
07:30:11.12 +70:04:13.8 -- not a known variable star
07:31:13.74 +69:47:28.7 -- not a known variable star
07:31:15.47 +69:55:49.9 -- not a known variable star
07:31:17.48 +69:44:00.9 -- not a known variable star
07:31:52.23 +70:11:36.1 -- not a known variable star
07:32:12.40 +70:18:03.1 -- not a known variable star
07:32:24.75 +69:11:44.5 -- not a known variable star
07:32:33.46 +69:38:25.7 -- not a known variable star
07:32:47.31 +69:15:22.5 -- not a known variable star
07:33:09.72 +70:11:16.3 -- not a known variable star
07:33:34.86 +69:52:19.8 -- not a known variable star
07:33:57.63 +69:22:08.1 -- not a known variable star
07:34:41.64 +69:41:54.1 -- not a known variable star
07:35:13.42 +69:25:02.4 -- not a known variable star
07:36:53.59 +69:19:06.4 -- not a known variable star
07:37:20.61 +70:05:24.9 -- not a known variable star
07:37:23.16 +70:46:07.2 -- not a known variable star
07:37:45.49 +69:50:39.7 -- a known variable star
07:38:07.17 +70:11:47.8 -- not a known variable star
07:38:36.42 +69:26:06.2 -- not a known variable star
07:38:46.17 +69:50:37.7 -- not a known variable star
07:40:20.28 +70:57:34.0 -- not a known variable star
07:40:32.80 +70:45:07.3 -- a known variable star
07:41:33.28 +70:58:55.4 -- not a known variable star
07:42:02.95 +69:30:29.5 -- not a known variable star
07:42:38.33 +69:52:50.6 -- not a known variable star
07:42:51.67 +70:09:15.2 -- not a known variable star
07:43:22.88 +70:28:54.4 -- not a known variable star
07:44:46.41 +70:58:43.7 -- not a known variable star
07:44:52.41 +70:02:49.3 -- not a known variable star
07:45:01.61 +70:12:41.6 -- not a known variable star
07:45:09.50 +70:46:39.3 -- not a known variable star
07:46:21.87 +70:12:43.5 -- not a known variable star
07:46:31.52 +70:42:00.2 -- a known variable star
07:47:18.35 +70:29:00.4 -- not a known variable star
07:47:20.20 +70:59:07.8 -- not a known variable star
07:49:43.74 +71:09:47.2 -- not a known variable star
07:49:58.51 +70:50:27.8 -- not a known variable star
07:51:14.18 +70:48:26.0 -- not a known variable star
07:51:30.71 +70:06:02.4 -- not a known variable star
07:51:40.73 +70:05:38.0 -- not a known variable star
07:52:15.54 +70:09:55.5 -- a known variable star
07:52:25.44 +71:01:40.1 -- not a known variable star
07:53:34.49 +70:07:40.2 -- not a known variable star
07:54:58.91 +70:56:17.9 -- not a known variable star
07:55:42.65 +70:47:35.4 -- not a known variable star
07:56:32.17 +70:28:04.7 -- not a known variable star
08:00:48.29 +71:04:00.7 -- not a known variable star
08:01:22.23 +71:09:08.3 -- a known variable star
08:06:24.51 +71:24:54.0 -- not a known variable star
Found 139 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
157 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 157 (excluding asteroids and hot pixels, 139 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)2461258.80534640 -observatory V36
07:46:07.12 +20:23:19.0 Mercury (-0.3mag)
11:55:59.66 -00:06:31.4 Venus (-4.3mag)
05:43:41.53 +23:32:50.2 Mars (1.3mag)
08:41:12.82 +18:47:41.0 Jupiter (-1.8mag)
00:56:32.67 +03:16:43.7 Saturn (0.6mag)
04:11:30.35 +20:56:22.2 Uranus (5.8mag)
00:16:12.52 +00:13:56.7 Neptune (7.7mag)
20:28:19.50 -23:29:26.3 Pluto (14.4mag)
02:52:06.12 +21:07:41.8 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 02:43 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461258.80534640:
08:41:18.61 +18:47:16.2 Io (6.0mag)
08:41:08.28 +18:48:01.1 Europa (6.3mag)
08:41:10.49 +18:47:55.0 Ganymede (5.6mag)
08:40:59.83 +18:48:39.8 Callisto (6.7mag)
08:38:48.61 +18:45:54.1 Himalia (15.7mag)
08:41:11.35 +18:47:47.9 Thebe (16.6mag)
08:38:19.30 +18:44:48.3 Elara (17.7mag)
08:45:18.77 +18:28:03.3 Pasiphae (17.9mag)
08:44:31.30 +18:57:32.6 Carme (19.0mag)
00:56:30.01 +03:17:10.7 Titan (8.4mag)
00:56:26.75 +03:16:46.1 Rhea (9.7mag)
00:56:36.54 +03:15:06.8 Iapetus (11.1mag)
00:56:19.07 +03:16:57.2 Hyperion (14.4mag)
00:55:57.58 +03:10:09.7 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 02:43 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.80534640:
18:55:29.31 -24:00:09.4 JWST
17:18:46.60 +39:35:09.2 Chandra
10:08:04.04 -56:36:34.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 02:43 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.80534640 -observatory V36
03:11:29.23 +17:12:53.7 17.7mag P/1996 R2 (Lagerkvist)
18:02:22.80 -34:38:22.0 14.0mag P/2010 H2 (Vales)
06:51:59.81 -68:49:50.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:18.44 +32:57:11.6 17.7mag C/2017 K2 (PANSTARRS)
03:37:58.91 +36:46:27.8 16.7mag P/2021 N1 (ZTF)
22:40:12.59 +31:33:39.5 17.3mag C/2022 E2 (ATLAS)
06:41:34.02 +26:34:26.5 16.8mag C/2022 N2 (PANSTARRS)
10:19:47.65 +28:33:21.3 17.0mag C/2022 QE78 (ATLAS)
09:27:34.48 +05:17:44.4 17.9mag C/2022 R6 (PANSTARRS)
15:12:09.91 -12:12:39.9 17.9mag P/2023 B1 (PANSTARRS)
21:13:18.17 +66:13:24.1 17.9mag C/2023 H5 (Lemmon)
15:49:48.92 -12:45:24.5 14.3mag C/2023 R1 (PANSTARRS)
08:05:55.96 +31:15:34.2 15.2mag C/2024 E1 (Wierzchos)
15:07:16.84 +15:36:57.8 17.7mag C/2024 G6 (ATLAS)
19:05:33.87 +42:58:02.0 13.7mag C/2024 J3 (ATLAS)
21:13:32.75 +49:05:03.6 17.6mag C/2024 R4 (PANSTARRS)
05:13:35.47 -12:59:34.2 15.5mag C/2024 T5 (ATLAS)
06:54:58.29 +24:29:36.7 17.9mag C/2025 J1 (Borisov)
07:29:59.24 -15:52:41.1 17.7mag C/2025 R3 (PANSTARRS)
10:30:14.40 +21:01:33.6 17.3mag C/2025 V2 (Rankin)
12:56:59.32 +02:28:36.1 17.0mag C/2025 Y1 (ATLAS)
16:03:39.71 +78:00:38.8 16.8mag C/2026 A2 (Bok)
03:06:45.13 +46:08:50.3 17.1mag C/2026 B2 (Sun-Gao)
11:45:12.89 +08:20:29.7 17.3mag A/2026 E1
21:56:12.00 -26:29:31.5 6.9mag 10P/Tempel
11:27:48.95 -03:16:53.1 16.2mag 29P/Schwassmann-Wachmann
04:36:51.65 +32:16:11.4 18.0mag 47P/Ashbrook-Jackson
11:03:46.60 +05:16:11.3 17.2mag 63P/Wild
00:54:17.80 -05:22:52.6 15.4mag 65P/Gunn
05:31:11.38 +20:43:43.2 13.7mag 78P/Gehrels
20:39:42.87 -23:18:06.5 17.8mag 84P/Giclas
02:58:48.62 +13:32:46.5 16.7mag 88P/Howell
07:50:58.55 +27:55:04.0 16.1mag 93P/Lovas
04:00:57.60 +16:07:41.9 17.6mag 112P/Urata-Niijima
05:50:08.44 +30:30:25.7 16.3mag 114P/Wiseman-Skiff
09:13:56.57 +26:58:21.0 15.0mag 123P/West-Hartley
11:39:53.81 -09:31:47.3 17.1mag 124P/Mrkos
05:33:43.18 +21:11:10.4 16.1mag 128P/Shoemaker-Holt
06:25:13.57 +18:59:32.9 17.9mag 131P/Mueller
00:03:41.16 +03:25:20.1 17.6mag 139P/Vaisala-Oterma
03:21:32.95 -19:44:43.6 14.0mag 161P/Hartley-IRAS
07:09:31.50 +37:41:42.2 15.8mag 162P/SidingSpring
15:48:31.06 +39:33:30.9 12.3mag 169P/NEAT
02:39:27.63 +09:28:39.0 17.6mag 220P/McNaught
16:40:37.57 -09:57:00.8 17.7mag 235P/LINEAR
20:23:40.07 -52:50:57.1 17.8mag 259P/Garradd
03:16:31.39 +24:21:17.9 15.4mag 260P/McNaught
06:59:35.10 +37:45:13.0 17.3mag 295P/LINEAR
15:09:52.41 +03:21:00.0 17.7mag 391P/Kowalski
08:59:08.17 +18:28:12.2 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 02:43 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
-rw-r--r-- 1 apache apache 189K Aug 6 02:43 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:39:31.292 -08:28:35.35 AT 2026vla 2026-02-21.40 20.65
17:07:24.157 +32:28:59.94 AT 2026vkz 2026-06-16.33 21.89
18:55:34.805 +34:42:05.78 AT 2026vky 2026-06-22.39 21.01
15:27:13.875 -10:50:21.14 AT 2026vkx 2026-06-14.35 20.55
13:36:43.476 +25:28:01.16 AT 2026vkw 2026-06-25.38 20.6
04:43:04.292 -16:08:54.64 AT 2026vkv 2026-01-12.30 21.72
04:48:25.928 -18:19:58.05 AT 2026vku 2026-01-26.25 21.35
12:55:24.686 +13:58:33.13 AT 2026vkt 2026-06-05.34 21.42
11:39:28.884 +47:23:59.43 AT 2026vks 2026-01-14.61 21.82
10:26:55.799 -14:09:20.42 AT 2026vkr 2026-01-13.55 21.98
12:26:22.284 +20:06:25.68 AT 2026vkq 2026-02-13.60 20.86
12:08:12.778 +41:30:56.83 AT 2026vkp 2026-06-15.27 20.88
05:11:50.298 -12:02:24.75 AT 2026vko 2026-02-15.23 20.49
00:35:37.087 -45:29:22.45 AT 2026vkn 2026-06-26.42 23.13
04:11:06.535 -49:23:35.67 AT 2026vkm 2026-07-09.42 22.31
23:40:19.411 -26:01:53.34 AT 2026vkl 2026-07-20.59 21.47
22:23:27.160 +00:54:32.97 AT 2026vkk 2026-07-14.55 21.17
21:14:05.875 -09:55:36.50 AT 2026vkj 2026-07-20.46 21.9
17:17:56.970 +19:09:32.22 AT 2026vki 2026-07-19.39 21.8
17:18:18.165 +24:21:20.44 AT 2026vkh 2026-07-19.40 21.78
-rw-r--r-- 1 apache apache 87K Aug 6 02:43 tns_transients_list.txt
