This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM
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 06.2001 2461258.7001 12.72 12:00:05.95 +60:41:34.5
133.94994 55.32354 galactic UMa Second-epoch detections are separated by 2.0" and 6.5 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 | 12:00:05.95 +60:41:34.5 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.037 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:05.95 +60:41:34.5: 13.90 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:05.95 +60:41:34.5: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 00 05.95 +60 41 34.5 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.74 11:54:44.99 +61:23:53.4
134.55671 54.43213 galactic UMa 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 | 11:54:44.99 +61:23:53.4 (user input) | T | P | (position from user input) J-Ks=0.732+/-0.046 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:54:44.99 +61:23:53.4: 14.03 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:54:44.99 +61:23:53.4: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 54 44.99 +61 23 53.4 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.74CV 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 06.2001 2461258.7001 11.34 11:51:43.96 +61:21:33.9
135.15511 54.32921 galactic UMa Second-epoch detections are separated by 0.3" 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 | Gaia DR3 859767485322263296 | 11:51:44.01 +61:21:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.469+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:51:43.96 +61:21:33.9: 12.24 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:51:43.96 +61:21:33.9: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 51 43.96 +61 21 33.9 11.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 859767485322263296,2461258.7001,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 859767485322263296 20260806.2001 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 11.64 11:55:34.58 +61:13:21.6
134.51086 54.63196 galactic UMa Second-epoch detections are separated by 0.3" 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 | Gaia DR3 859026551924086528 | 11:55:34.55 +61:13:21.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.389+/-0.030 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:34.58 +61:13:21.6: 12.59 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:34.58 +61:13:21.6: 12.61 +/- 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!
TCP 2026 08 06.2001* 11 55 34.58 +61 13 21.6 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 859026551924086528,2461258.7001,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 859026551924086528 20260806.2001 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 06.2001 2461258.7001 11.90 11:58:45.17 +60:51:43.4
134.11558 55.10749 galactic UMa Second-epoch detections are separated by 0.9" 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 | 11:58:45.17 +60:51:43.4 (user input) | T | P | (position from user input) J-Ks=0.209+/-0.029 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:45.17 +60:51:43.4: 12.80 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:45.17 +60:51:43.4: 12.87 +/- 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!
TCP 2026 08 06.2001* 11 58 45.17 +60 51 43.4 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 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 06.2001 2461258.7001 11.94 11:56:49.64 +61:41:58.6
133.97214 54.24255 galactic UMa Second-epoch detections are separated by 0.7" 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 | 11:56:49.64 +61:41:58.6 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.027 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:56:49.64 +61:41:58.6: 12.84 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:56:49.64 +61:41:58.6: 12.86 +/- 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!
TCP 2026 08 06.2001* 11 56 49.64 +61 41 58.6 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 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 06.2001 2461258.7001 12.10 11:52:36.83 +61:31:52.9
134.87430 54.21190 galactic UMa Second-epoch detections are separated by 2.2" 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 | 11:52:36.83 +61:31:52.9 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.027 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:36.83 +61:31:52.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:36.83 +61:31:52.9: 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!
TCP 2026 08 06.2001* 11 52 36.83 +61 31 52.9 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.12 12:00:35.01 +61:02:21.1
133.64413 55.01878 galactic UMa Second-epoch detections are separated by 1.1" 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 | 12:00:35.01 +61:02:21.1 (user input) | T | P | (position from user input) J-Ks=0.559+/-0.031 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:35.01 +61:02:21.1: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:35.01 +61:02:21.1: 13.09 +/- 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!
TCP 2026 08 06.2001* 12 00 35.01 +61 02 21.1 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 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 06.2001 2461258.7001 12.19 11:59:44.42 +61:16:43.9
133.66711 54.75878 galactic UMa Second-epoch detections are separated by 1.2" 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 | 11:59:44.42 +61:16:43.9 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:44.42 +61:16:43.9: 13.21 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:44.42 +61:16:43.9: 13.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 59 44.42 +61 16 43.9 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.36 12:06:47.05 +61:26:17.0
132.19125 54.88018 galactic UMa Second-epoch detections are separated by 1.4" and 6.5 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 | 12:06:47.05 +61:26:17.0 (user input) | T | P | (position from user input) J-Ks=0.485+/-0.035 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:06:47.05 +61:26:17.0: 13.27 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:06:47.05 +61:26:17.0: 13.23 +/- 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!
TCP 2026 08 06.2001* 12 06 47.05 +61 26 17.0 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.44 11:52:19.49 +59:15:07.6
136.52211 56.28911 galactic UMa Second-epoch detections are separated by 1.8" and 6.4 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 | 11:52:19.49 +59:15:07.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.401+/-0.031 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:19.49 +59:15:07.6: 13.30 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:19.49 +59:15:07.6: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 52 19.49 +59 15 07.6 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.48 12:55:18.70 +66:06:13.2
122.30830 51.01989 galactic Dra Second-epoch detections are separated by 0.8" and 6.7 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 | 12:55:18.70 +66:06:13.2 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.036 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:55:18.70 +66:06:13.2: 13.36 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:55:18.70 +66:06:13.2: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.43 11:53:12.33 +61:35:12.0
134.72678 54.18791 galactic UMa Second-epoch detections are separated by 0.5" 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 | 11:53:12.33 +61:35:12.0 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.028 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:53:12.33 +61:35:12.0: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:53:12.33 +61:35:12.0: 13.43 +/- 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!
TCP 2026 08 06.2001* 11 53 12.33 +61 35 12.0 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.51 11:49:53.56 +61:07:32.2
135.66403 54.45508 galactic UMa 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 | 11:49:53.56 +61:07:32.2 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.029 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:49:53.56 +61:07:32.2: 13.49 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:49:53.56 +61:07:32.2: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 49 53.56 +61 07 32.2 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.53 11:57:17.91 +60:23:42.6
134.70369 55.47851 galactic UMa Second-epoch detections are separated by 1.1" 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 | 11:57:17.91 +60:23:42.6 (user input) | T | P | (position from user input) J-Ks=0.308+/-0.033 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:17.91 +60:23:42.6: 13.60 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:17.91 +60:23:42.6: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 57 17.91 +60 23 42.6 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.62 12:03:11.87 +60:49:03.7
133.24966 55.33370 galactic UMa Second-epoch detections are separated by 0.8" and 6.5 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 | 12:03:11.87 +60:49:03.7 (user input) | T | P | (position from user input) J-Ks=0.525+/-0.032 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:03:11.87 +60:49:03.7: 13.71 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:03:11.87 +60:49:03.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 03 11.87 +60 49 03.7 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.67 13:08:38.85 +64:09:44.5
119.82752 52.86203 galactic Dra Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:08:38.85 +64:09:44.5 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.032 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 13:08:38.85 +64:09:44.5: 13.67 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 13:08:38.85 +64:09:44.5: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.67CV 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 06.2001 2461258.7001 12.62 11:55:10.57 +61:27:26.8
134.43743 54.39615 galactic UMa Second-epoch detections are separated by 1.4" 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 | 11:55:10.57 +61:27:26.8 (user input) | T | P | (position from user input) J-Ks=0.530+/-0.030 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:10.57 +61:27:26.8: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:10.57 +61:27:26.8: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 55 10.57 +61 27 26.8 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.74 12:16:32.45 +59:27:21.8
131.09396 57.11577 galactic UMa Second-epoch detections are separated by 1.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:16:32.45 +59:27:21.8 (user input) | T | P | (position from user input) J-Ks=0.569+/-0.033 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:16:32.45 +59:27:21.8: 13.70 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:16:32.45 +59:27:21.8: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 16 32.45 +59 27 21.8 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.74CV 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 06.2001 2461258.7001 12.58 11:52:36.94 +61:32:42.9
134.86478 54.19917 galactic UMa Second-epoch detections are separated by 2.4" and 6.6 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 | 11:52:36.94 +61:32:42.9 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.029 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:36.94 +61:32:42.9: 13.66 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:36.94 +61:32:42.9: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 52 36.94 +61 32 42.9 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.62 12:01:10.92 +61:10:44.3
133.44307 54.91182 galactic UMa Second-epoch detections are separated by 2.5" 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 | 12:01:10.92 +61:10:44.3 (user input) | T | P | (position from user input) J-Ks=0.282+/-0.035 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:10.92 +61:10:44.3: 13.64 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:10.92 +61:10:44.3: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 01 10.92 +61 10 44.3 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.55 11:53:41.22 +61:37:52.7
134.60731 54.16843 galactic UMa Second-epoch detections are separated by 1.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:53:41.22 +61:37:52.7 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:53:41.22 +61:37:52.7: 13.64 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:53:41.22 +61:37:52.7: 13.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 53 41.22 +61 37 52.7 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.62 11:59:05.14 +60:12:29.1
134.45866 55.73314 galactic UMa Second-epoch detections are separated by 1.6" and 6.5 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 | 11:59:05.14 +60:12:29.1 (user input) | T | P | (position from user input) J-Ks=0.723+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:05.14 +60:12:29.1: 13.63 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:05.14 +60:12:29.1: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 59 05.14 +60 12 29.1 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.64 12:02:28.79 +60:48:44.0
133.39809 55.31005 galactic UMa Second-epoch detections are separated by 2.2" and 6.7 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 | 12:02:28.79 +60:48:44.0 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.035 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:28.79 +60:48:44.0: 13.63 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:28.79 +60:48:44.0: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 02 28.79 +60 48 44.0 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.64CV 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 06.2001 2461258.7001 12.51 12:00:42.25 +60:52:53.8
133.71423 55.17188 galactic UMa Second-epoch detections are separated by 1.9" and 6.6 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 | 12:00:42.25 +60:52:53.8 (user input) | T | P | (position from user input) J-Ks=0.571+/-0.031 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:42.25 +60:52:53.8: 13.60 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:42.25 +60:52:53.8: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 00 42.25 +60 52 53.8 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.54 11:48:59.38 +61:39:18.9
135.46487 53.92723 galactic UMa Second-epoch detections are separated by 2.4" and 6.0 pix
The object was found in VSX 1" Gaia DR3 859757349199468800
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.450 G 13.480 G F
The object was not found in astcheck.
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:48:59.38 +61:39:18.9: 13.61 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:48:59.38 +61:39:18.9: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 48 59.38 +61 39 18.9 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 859757349199468800,2461258.7001,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 859757349199468800 20260806.2001 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.57 12:03:56.13 +60:43:07.7
133.15627 55.45649 galactic UMa Second-epoch detections are separated by 0.4" 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 | 12:03:56.13 +60:43:07.7 (user input) | T | P | (position from user input) J-Ks=0.697+/-0.033 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:03:56.13 +60:43:07.7: 13.59 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:03:56.13 +60:43:07.7: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 03 56.13 +60 43 07.7 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.68 12:15:16.78 +58:59:23.1
131.60275 57.52565 galactic UMa Second-epoch detections are separated by 0.2" and 6.6 pix
The object was found in VSX 1" Gaia DR3 1575888135866281088
Type: ROT
# Max. Min./Amp. JD0 Period
13.270 G 13.300 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:15:16.78 +58:59:23.1: 13.60 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:15:16.78 +58:59:23.1: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 15 16.78 +58 59 23.1 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1575888135866281088,2461258.7001,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1575888135866281088 20260806.2001 12.68CV 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 06.2001 2461258.7001 12.62 12:01:21.35 +60:36:38.0
133.74524 55.45383 galactic UMa Second-epoch detections are separated by 1.0" and 6.4 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 | 12:01:21.35 +60:36:38.0 (user input) | T | P | (position from user input) J-Ks=0.475+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:21.35 +60:36:38.0: 13.57 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:21.35 +60:36:38.0: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 01 21.35 +60 36 38.0 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.39 11:58:43.93 +61:21:06.0
133.81959 54.64844 galactic UMa Second-epoch detections are separated by 2.1" and 6.4 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 | 11:58:43.93 +61:21:06.0 (user input) | T | P | (position from user input) J-Ks=0.278+/-0.033 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:43.93 +61:21:06.0: 13.57 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:43.93 +61:21:06.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 58 43.93 +61 21 06.0 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.52 11:59:07.58 +61:41:41.8
133.53802 54.34298 galactic UMa Second-epoch detections are separated by 0.5" 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 | 11:59:07.58 +61:41:41.8 (user input) | T | P | (position from user input) J-Ks=0.519+/-0.031 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:07.58 +61:41:41.8: 13.52 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:07.58 +61:41:41.8: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 59 07.58 +61 41 41.8 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.34 11:54:37.54 +61:07:21.9
134.75922 54.68171 galactic UMa Second-epoch detections are separated by 0.7" 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 | 11:54:37.54 +61:07:21.9 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.032 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:54:37.54 +61:07:21.9: 13.49 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:54:37.54 +61:07:21.9: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 54 37.54 +61 07 21.9 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.46 12:02:20.75 +61:50:48.9
132.83548 54.32731 galactic UMa Second-epoch detections are separated by 1.3" 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 | 12:02:20.75 +61:50:48.9 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.032 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:20.75 +61:50:48.9: 13.49 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:20.75 +61:50:48.9: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 02 20.75 +61 50 48.9 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.49 12:19:10.03 +59:58:32.3
130.27853 56.68994 galactic UMa Second-epoch detections are separated by 0.8" 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 | 12:19:10.03 +59:58:32.3 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.029 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:19:10.03 +59:58:32.3: 13.49 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:19:10.03 +59:58:32.3: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 19 10.03 +59 58 32.3 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.55 12:06:17.19 +61:23:58.8
132.31004 54.89885 galactic UMa Second-epoch detections are separated by 0.9" 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 | 12:06:17.19 +61:23:58.8 (user input) | T | P | (position from user input) J-Ks=0.670+/-0.030 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:06:17.19 +61:23:58.8: 13.47 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:06:17.19 +61:23:58.8: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 06 17.19 +61 23 58.8 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.58 12:53:59.14 +66:04:42.2
122.52111 51.04783 galactic Dra Second-epoch detections are separated by 1.1" and 6.7 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 | 12:53:59.14 +66:04:42.2 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:53:59.14 +66:04:42.2: 13.45 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:53:59.14 +66:04:42.2: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.52 12:02:58.64 +61:29:47.4
132.90880 54.68310 galactic UMa Second-epoch detections are separated by 0.5" 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 | 12:02:58.64 +61:29:47.4 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.034 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:58.64 +61:29:47.4: 13.45 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:58.64 +61:29:47.4: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 02 58.64 +61 29 47.4 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.49 12:02:09.39 +60:49:57.6
133.45143 55.27767 galactic UMa Second-epoch detections are separated by 0.2" 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 | 12:02:09.39 +60:49:57.6 (user input) | T | P | (position from user input) J-Ks=0.312+/-0.033 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:09.39 +60:49:57.6: 13.45 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:09.39 +60:49:57.6: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 02 09.39 +60 49 57.6 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.30 11:54:58.09 +61:08:36.8
134.67943 54.67800 galactic UMa Second-epoch detections are separated by 0.8" 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 | 11:54:58.09 +61:08:36.8 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.032 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:54:58.09 +61:08:36.8: 13.46 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:54:58.09 +61:08:36.8: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 54 58.09 +61 08 36.8 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.46 11:51:54.89 +61:18:35.0
135.15414 54.38349 galactic UMa Second-epoch detections are separated by 1.1" 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 | 11:51:54.89 +61:18:35.0 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.028 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:51:54.89 +61:18:35.0: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:51:54.89 +61:18:35.0: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 51 54.89 +61 18 35.0 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.46 12:01:48.36 +61:24:12.8
133.19031 54.72515 galactic UMa Second-epoch detections are separated by 1.8" and 6.4 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 | 12:01:48.36 +61:24:12.8 (user input) | T | P | (position from user input) J-Ks=0.520+/-0.030 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:48.36 +61:24:12.8: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:48.36 +61:24:12.8: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 01 48.36 +61 24 12.8 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.39 11:57:32.62 +61:24:16.4
134.01704 54.54858 galactic UMa Second-epoch detections are separated by 0.4" 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 | 11:57:32.62 +61:24:16.4 (user input) | T | P | (position from user input) J-Ks=0.681+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:32.62 +61:24:16.4: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:32.62 +61:24:16.4: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 57 32.62 +61 24 16.4 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.42 12:00:34.89 +61:25:21.9
133.41798 54.65801 galactic UMa Second-epoch detections are separated by 0.7" and 6.4 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 | 12:00:34.89 +61:25:21.9 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.031 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:34.89 +61:25:21.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:34.89 +61:25:21.9: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 00 34.89 +61 25 21.9 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.37 11:52:44.62 +61:01:48.6
135.18414 54.67985 galactic UMa Second-epoch detections are separated by 1.0" 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 | 11:52:44.62 +61:01:48.6 (user input) | T | P | (position from user input) J-Ks=0.570+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:44.62 +61:01:48.6: 13.38 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:44.62 +61:01:48.6: 13.42 +/- 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!
TCP 2026 08 06.2001* 11 52 44.62 +61 01 48.6 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.36 11:57:46.45 +60:41:41.4
134.41568 55.22082 galactic UMa Second-epoch detections are separated by 1.7" 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 | 11:57:46.45 +60:41:41.4 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.030 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:46.45 +60:41:41.4: 13.36 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:46.45 +60:41:41.4: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 57 46.45 +60 41 41.4 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.41 12:00:29.21 +60:51:19.3
133.77351 55.18746 galactic UMa Second-epoch detections are separated by 0.6" 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 | 12:00:29.21 +60:51:19.3 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.032 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:29.21 +60:51:19.3: 13.34 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:29.21 +60:51:19.3: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 00 29.21 +60 51 19.3 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.41 11:55:28.62 +61:57:44.1
134.06305 53.94001 galactic UMa Second-epoch detections are separated by 2.6" 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 | 11:55:28.62 +61:57:44.1 (user input) | T | P | (position from user input) J-Ks=0.340+/-0.031 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:28.62 +61:57:44.1: 13.35 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:28.62 +61:57:44.1: 13.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 55 28.62 +61 57 44.1 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.37 12:01:02.31 +61:10:14.4
133.47627 54.91380 galactic UMa Second-epoch detections are separated by 1.1" and 6.5 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 | 12:01:02.31 +61:10:14.4 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:02.31 +61:10:14.4: 13.34 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:02.31 +61:10:14.4: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 01 02.31 +61 10 14.4 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.35 11:55:13.87 +61:37:05.8
134.32478 54.24921 galactic UMa Second-epoch detections are separated by 1.0" 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 | 11:55:13.87 +61:37:05.8 (user input) | T | P | (position from user input) J-Ks=0.606+/-0.030 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:13.87 +61:37:05.8: 13.31 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:13.87 +61:37:05.8: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 55 13.87 +61 37 05.8 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.31 12:01:50.61 +61:00:37.1
133.41040 55.09752 galactic UMa Second-epoch detections are separated by 0.8" 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 | 12:01:50.61 +61:00:37.1 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.033 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:50.61 +61:00:37.1: 13.31 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:50.61 +61:00:37.1: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 01 50.61 +61 00 37.1 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.40 11:59:03.34 +61:30:44.9
133.66023 54.51124 galactic UMa Second-epoch detections are separated by 1.1" 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 | 11:59:03.34 +61:30:44.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:03.34 +61:30:44.9: 13.30 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:03.34 +61:30:44.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 59 03.34 +61 30 44.9 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.29 11:49:38.18 +60:59:54.9
135.80196 54.55844 galactic UMa Second-epoch detections are separated by 1.9" and 6.4 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 | 11:49:38.18 +60:59:54.9 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.030 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:49:38.18 +60:59:54.9: 13.27 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:49:38.18 +60:59:54.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 49 38.18 +60 59 54.9 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.27 12:02:34.21 +62:05:01.9
132.66197 54.11156 galactic UMa Second-epoch detections are separated by 0.4" and 6.4 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 | 12:02:34.21 +62:05:01.9 (user input) | T | P | (position from user input) J-Ks=0.532+/-0.031 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:34.21 +62:05:01.9: 13.19 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:34.21 +62:05:01.9: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 02 34.21 +62 05 01.9 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.13 11:50:58.06 +61:23:41.4
135.27533 54.26046 galactic UMa Second-epoch detections are separated by 0.5" 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 | 11:50:58.06 +61:23:41.4 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.030 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:50:58.06 +61:23:41.4: 13.18 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:50:58.06 +61:23:41.4: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 50 58.06 +61 23 41.4 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.22 11:58:44.41 +61:35:58.0
133.66875 54.41663 galactic UMa Second-epoch detections are separated by 0.4" 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 | 11:58:44.41 +61:35:58.0 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.030 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:44.41 +61:35:58.0: 13.16 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:44.41 +61:35:58.0: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 58 44.41 +61 35 58.0 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.10 11:57:23.19 +61:19:57.2
134.09188 54.60905 galactic UMa Second-epoch detections are separated by 1.4" 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 | 11:57:23.19 +61:19:57.2 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.031 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:23.19 +61:19:57.2: 13.16 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:23.19 +61:19:57.2: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 57 23.19 +61 19 57.2 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.23 11:49:22.81 +61:33:39.9
135.45775 54.03213 galactic UMa Second-epoch detections are separated by 1.6" 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 | 11:49:22.81 +61:33:39.9 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.029 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:49:22.81 +61:33:39.9: 13.13 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:49:22.81 +61:33:39.9: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 49 22.81 +61 33 39.9 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.18 11:59:15.68 +61:17:13.9
133.75562 54.73102 galactic UMa Second-epoch detections are separated by 1.2" 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 | 11:59:15.68 +61:17:13.9 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:15.68 +61:17:13.9: 13.13 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:15.68 +61:17:13.9: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 59 15.68 +61 17 13.9 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.15 11:55:58.80 +60:47:59.6
134.70484 55.04263 galactic UMa Second-epoch detections are separated by 0.9" 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 | 11:55:58.80 +60:47:59.6 (user input) | T | P | (position from user input) J-Ks=0.485+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:58.80 +60:47:59.6: 13.13 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:58.80 +60:47:59.6: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 55 58.80 +60 47 59.6 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.04 11:57:00.91 +61:00:01.3
134.37237 54.90258 galactic UMa Second-epoch detections are separated by 0.5" 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 | 11:57:00.91 +61:00:01.3 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.031 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:00.91 +61:00:01.3: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:00.91 +61:00:01.3: 13.08 +/- 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!
TCP 2026 08 06.2001* 11 57 00.91 +61 00 01.3 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 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 06.2001 2461258.7001 12.12 11:49:00.81 +61:00:55.1
135.90873 54.51220 galactic UMa Second-epoch detections are separated by 1.2" 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 | 11:49:00.81 +61:00:55.1 (user input) | T | P | (position from user input) J-Ks=0.585+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:49:00.81 +61:00:55.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:49:00.81 +61:00:55.1: 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!
TCP 2026 08 06.2001* 11 49 00.81 +61 00 55.1 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 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 06.2001 2461258.7001 11.98 12:00:44.15 +61:24:53.3
133.39259 54.67173 galactic UMa Second-epoch detections are separated by 0.8" 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 | 12:00:44.15 +61:24:53.3 (user input) | T | P | (position from user input) J-Ks=0.548+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:44.15 +61:24:53.3: 12.88 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:44.15 +61:24:53.3: 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!
TCP 2026 08 06.2001* 12 00 44.15 +61 24 53.3 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 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 06.2001 2461258.7001 11.88 11:55:22.27 +61:27:51.9
134.39584 54.39832 galactic UMa Second-epoch detections are separated by 1.1" 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 | 11:55:22.27 +61:27:51.9 (user input) | T | P | (position from user input) J-Ks=0.224+/-0.033 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:22.27 +61:27:51.9: 12.87 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:22.27 +61:27:51.9: 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!
TCP 2026 08 06.2001* 11 55 22.27 +61 27 51.9 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 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 06.2001 2461258.7001 11.92 11:55:09.20 +61:20:51.6
134.51204 54.49703 galactic UMa Second-epoch detections are separated by 1.3" 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 | 11:55:09.20 +61:20:51.6 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.031 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:09.20 +61:20:51.6: 12.86 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:09.20 +61:20:51.6: 12.89 +/- 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!
TCP 2026 08 06.2001* 11 55 09.20 +61 20 51.6 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 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 06.2001 2461258.7001 11.82 11:58:13.08 +61:06:51.8
134.06506 54.84858 galactic UMa Second-epoch detections are separated by 0.7" 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 | 11:58:13.08 +61:06:51.8 (user input) | T | P | (position from user input) J-Ks=0.321+/-0.028 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:13.08 +61:06:51.8: 12.77 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:13.08 +61:06:51.8: 12.73 +/- 0.01 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!
TCP 2026 08 06.2001* 11 58 13.08 +61 06 51.8 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 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 06.2001 2461258.7001 11.57 12:01:09.64 +61:41:15.9
133.15259 54.43156 galactic UMa Second-epoch detections are separated by 0.4" 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 | Gaia DR3 1582448062755566848 | 12:01:09.66 +61:41:15.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.313+/-0.030 (F)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:09.64 +61:41:15.9: 12.48 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:09.64 +61:41:15.9: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 01 09.64 +61 41 15.9 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1582448062755566848,2461258.7001,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1582448062755566848 20260806.2001 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.95 11:55:03.10 +60:57:56.1
134.77917 54.84671 galactic UMa Second-epoch detections are separated by 0.3" 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 | 11:55:03.10 +60:57:56.1 (user input) | T | P | (position from user input) J-Ks=0.331+/-0.034 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:03.10 +60:57:56.1: 14.23 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:03.10 +60:57:56.1: 14.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 55 03.10 +60 57 56.1 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.71 11:53:06.22 +61:16:03.2
134.95623 54.47788 galactic UMa Second-epoch detections are separated by 1.3" 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 | 11:53:06.22 +61:16:03.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:53:06.22 +61:16:03.2: 14.01 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:53:06.22 +61:16:03.2: 14.00 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 53 06.22 +61 16 03.2 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.71CV 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 06.2001 2461258.7001 12.79 11:56:16.14 +61:22:43.6
134.27829 54.51745 galactic UMa Second-epoch detections are separated by 2.0" 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 | 11:56:16.14 +61:22:43.6 (user input) | T | P | (position from user input) J-Ks=0.520+/-0.031 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:56:16.14 +61:22:43.6: 14.01 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:56:16.14 +61:22:43.6: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 56 16.14 +61 22 43.6 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.79 12:00:29.74 +60:21:33.9
134.07384 55.65320 galactic UMa Second-epoch detections are separated by 1.3" and 6.1 pix
The object was found in VSX 2" NSVS 2629927
Type: EB|EW
# Max. Min./Amp. JD0 Period
13.521 R1 13.944 R1 0.266712000000
The object was not found in astcheck.
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:29.74 +60:21:33.9: 13.96 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:29.74 +60:21:33.9: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 00 29.74 +60 21 33.9 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2629927,2461258.7001,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2629927 20260806.2001 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.68 11:56:11.42 +61:21:11.9
134.30946 54.53771 galactic UMa Second-epoch detections are separated by 1.1" 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 | 11:56:11.42 +61:21:11.9 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:56:11.42 +61:21:11.9: 13.90 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:56:11.42 +61:21:11.9: 13.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 56 11.42 +61 21 11.9 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.68CV 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 06.2001 2461258.7001 12.65 11:57:05.68 +61:09:39.4
134.25557 54.75646 galactic UMa Second-epoch detections are separated by 2.4" 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 | 11:57:05.68 +61:09:39.4 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.031 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:05.68 +61:09:39.4: 13.81 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:05.68 +61:09:39.4: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 57 05.68 +61 09 39.4 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.71 12:00:48.84 +61:00:46.9
133.61391 55.05290 galactic UMa Second-epoch detections are separated by 1.5" 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 | 12:00:48.84 +61:00:46.9 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:48.84 +61:00:46.9: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:48.84 +61:00:46.9: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 00 48.84 +61 00 46.9 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.71CV 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 06.2001 2461258.7001 12.76 12:20:36.17 +60:10:14.3
129.88257 56.53955 galactic UMa Second-epoch detections are separated by 1.1" and 6.7 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 | 12:20:36.17 +60:10:14.3 (user input) | T | P | (position from user input) J-Ks=0.534+/-0.026 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:20:36.17 +60:10:14.3: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:20:36.17 +60:10:14.3: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 12 20 36.17 +60 10 14.3 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.60 11:58:54.38 +60:59:32.4
134.00474 54.99222 galactic UMa Second-epoch detections are separated by 1.2" 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 | 11:58:54.38 +60:59:32.4 (user input) | T | P | (position from user input) J-Ks=0.556+/-0.033 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:54.38 +60:59:32.4: 13.75 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:54.38 +60:59:32.4: 13.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 58 54.38 +60 59 32.4 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2001 2461258.7001 12.59 11:52:17.28 +61:49:49.9
134.73824 53.92100 galactic UMa Second-epoch detections are separated by 1.1" 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 | 11:52:17.28 +61:49:49.9 (user input) | T | P | (position from user input) J-Ks=0.781+/-0.029 (K)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:17.28 +61:49:49.9: 13.72 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:17.28 +61:49:49.9: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2001* 11 52 17.28 +61 49 49.9 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7001,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2001 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.77304396 22.02.2026 06:33:00.998 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
First image: 2461093.77304396 22.02.2026 06:33:00.998 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Last image: 2461258.70061323 06.08.2026 04:48:42.983 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
JD time system (TT/UTC/UNKNOWN): UTC
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: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7055
Objects passed selection criteria: 7010
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 4435.25
Average stars matched: 4326.5 (97.5481 %)
Memory usage VmPeak: 233268 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 00:01:13 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: 2461093.77304396 22.02.2026 06:33:00.998 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
First image: 2461093.77304396 22.02.2026 06:33:00.998 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Last image: 2461258.70061323 06.08.2026 04:48:42.983 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 89
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 10 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): 35229
Objects passed selection criteria: 35106
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 23408.5
Average stars matched: 22530.2 (96.2482 %)
Memory usage VmPeak: 258080 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 00:02:08 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
SExtractor catalog cache: saved UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.cat to cache
SExtractor catalog cache: saved UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.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/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.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: 2461258.69955678
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_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits exists and is non-empty
Saving wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits to local_wcs_cache/
'wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits' -> 'local_wcs_cache/wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits'
wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits exists and is non-empty
Saving wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits to local_wcs_cache/
'wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits' -> 'local_wcs_cache/wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits'
wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits exists and is non-empty
Saving wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits to local_wcs_cache/
'wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits' -> 'local_wcs_cache/wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits'
wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits exists and is non-empty
Saving wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits to local_wcs_cache/
'wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits' -> 'local_wcs_cache/wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits (1st reference image)
verification OK: wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Image size: 941.9'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: 12:00:03.636 +62:00:23.32 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_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits (1st new image)
verification OK: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:00:40.208 +61:59:13.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:03.636 +62:00:23.32
Second-epoch image center 12:00:40.208 +61:59:13.43
Angular distance between the image centers 0.0741 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits (2nd new image)
verification OK: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:00:37.803 +61:58:40.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:03.636 +62:00:23.32
Second-epoch image center 12:00:37.803 +61:58:40.36
Angular distance between the image centers 0.0727 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 12:00:40.208 +61:59:13.43
Second-epoch second image center 12:00:37.803 +61:58:40.36
Angular distance between the image centers 0.01032 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/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits &> /tmp/tmp.ceSrp0KT4W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits &> /tmp/tmp.orsg6xhK32
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits &> /tmp/tmp.Tb5akJQphM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits &> /tmp/tmp.1AdRT3LH4Q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.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_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.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_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
Found non-empty wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
The reference image (wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits) and catalog (wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat) found
'wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat' -> 'wcsmag.cat'
Read 7332 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.9729 to 198.4317 deg, Dec +55.2640 to +67.4533 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 159.9729 to 198.4317 deg, Dec 55.2640 to 67.4533 deg
Loaded 6574 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): 3976 out of 4190 total matches.
Matched with Tycho-2 4190 out of 7332 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.896950
a=0.000000 b=1.000000 c=22.896950
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7332 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.9729 to 198.4317 deg, Dec +55.2640 to +67.4533 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 159.9729 to 198.4317 deg, Dec 55.2640 to 67.4533 deg
Loaded 6574 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): 3976 out of 4190 total matches.
Matched with Tycho-2 4190 out of 7332 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Forced-photometry filter: calibrated wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits -> calib.txt_param_ref_wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits (aperture=6.4)
Read 7282 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.9723 to 198.4317 deg, Dec +55.3313 to +67.4947 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 159.9723 to 198.4317 deg, Dec 55.3313 to 67.4947 deg
Loaded 6542 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): 3979 out of 4176 total matches.
Matched with Tycho-2 4176 out of 7282 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Forced-photometry filter: calibrated wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits -> calib.txt_param_ref_wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits (aperture=6.4)
____ 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:
2.2 pix UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
2.2 pix UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
2.7 pix fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
2.7 pix fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Limiting magnitude estimates:
15.4 mag. UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
15.4 mag. UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
13.1 mag. fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
12.6 mag. fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 10.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ceSrp0KT4W (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits' -> 'wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.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/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS_IMAGE_NAME=wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS-calibrated image found: wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Checking if the catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat corresponding to the image wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits alredy exist and is non-empty...
Catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat corresponding to the image wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS catalog name: wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=506, bad_region=0, passed=7332
Got 7332 stars (including 6822 good ones) from the SExtractor catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
util/solve_plate_with_UCAC5 got 7332 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 7332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 7332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 7332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4906 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits N_match=4906 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.437 sigma_q2_arcsec=0.363 sigma_q3_arcsec=0.338 sigma_q4_arcsec=0.320 n_q1=1138 n_q2=1153 n_q3=1306 n_q4=1309 worst_quadrant_to_overall_ratio=1.205
The image catalog is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits -region wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.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.orsg6xhK32 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits' -> 'wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.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/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS_IMAGE_NAME=wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS-calibrated image found: wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Checking if the catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat corresponding to the image wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits alredy exist and is non-empty...
Catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat corresponding to the image wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS catalog name: wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=494, bad_region=0, passed=7282
Got 7282 stars (including 6779 good ones) from the SExtractor catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat
util/solve_plate_with_UCAC5 got 7282 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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 7282 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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 7282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 7282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4906 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits N_match=4906 sigma_overall_arcsec=0.386 sigma_q1_arcsec=0.483 sigma_q2_arcsec=0.383 sigma_q3_arcsec=0.367 sigma_q4_arcsec=0.343 n_q1=1150 n_q2=1156 n_q3=1305 n_q4=1295 worst_quadrant_to_overall_ratio=1.252
The image catalog is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits -region wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.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.Tb5akJQphM (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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
WCS_IMAGE_NAME=wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
WCS-calibrated image found: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
Checking if the catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
WCS catalog name: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=60, bad_region=0, passed=1635
Got 1635 stars (including 1574 good ones) from the SExtractor catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat
util/solve_plate_with_UCAC5 got 1635 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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 1541 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1536 matched stars entering correct_measured_positions(), 1527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1536 matched stars entering correct_measured_positions(), 1623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 1543 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1537 matched stars entering correct_measured_positions(), 1623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 1537 matched stars entering correct_measured_positions(), 1623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 1537 stars left (next iteration limit 1689)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1537 robust_rms=6.644 arcsec worst_quadrant_rms=39.779 arcsec
SIP_REFIT: SIP order 3 trial: matched=1537 robust_rms=0.432 arcsec worst_quadrant_rms=0.539 arcsec
SIP_REFIT: SIP order 5 trial: matched=1537 robust_rms=0.335 arcsec worst_quadrant_rms=0.412 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1537 robust_rms_before=0.826 arcsec robust_rms_before_corrected=0.334 arcsec robust_rms_after=0.335 arcsec worst_quadrant_rms_before=0.441 worst_quadrant_rms_after=0.412
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.441 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits N_match=1537 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.316 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.305 sigma_q4_arcsec=0.373 n_q1=561 n_q2=315 n_q3=433 n_q4=228 worst_quadrant_to_overall_ratio=1.252
The image catalog is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits -region wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.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.1AdRT3LH4Q (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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
WCS_IMAGE_NAME=wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
WCS-calibrated image found: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Checking if the catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
WCS catalog name: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=53, bad_region=0, passed=1572
Got 1572 stars (including 1518 good ones) from the SExtractor catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
util/solve_plate_with_UCAC5 got 1572 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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 1483 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1482 matched stars entering correct_measured_positions(), 1470 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1482 matched stars entering correct_measured_positions(), 1555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 1484 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1482 matched stars entering correct_measured_positions(), 1554 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 1482 matched stars entering correct_measured_positions(), 1554 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 1482 stars left (next iteration limit 1630)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1482 robust_rms=7.086 arcsec worst_quadrant_rms=22.925 arcsec
SIP_REFIT: SIP order 3 trial: matched=1482 robust_rms=0.401 arcsec worst_quadrant_rms=0.458 arcsec
SIP_REFIT: SIP order 5 trial: matched=1482 robust_rms=0.316 arcsec worst_quadrant_rms=0.385 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1482 robust_rms_before=0.790 arcsec robust_rms_before_corrected=0.352 arcsec robust_rms_after=0.316 arcsec worst_quadrant_rms_before=0.436 worst_quadrant_rms_after=0.385
verification OK: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
verification OK: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Image size: 941.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:00:37.696 +61:58:40.09 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1572 stars ###
'wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/correct_sextractor_wcs_catalog_usingxy2sky2194940.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.790 -> 0.316 arcsec)
WCS_QUALITY_DIAG: file=fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits N_match=1482 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.283 sigma_q2_arcsec=0.401 sigma_q3_arcsec=0.293 sigma_q4_arcsec=0.389 n_q1=495 n_q2=319 n_q3=440 n_q4=228 worst_quadrant_to_overall_ratio=1.254
The image catalog is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits -region wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.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=UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits sigma_overall=0.363 worst_q_ratio=1.205
ref2=UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits sigma_overall=0.386 worst_q_ratio=1.252
new1=fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits sigma_overall=0.349 worst_q_ratio=1.252
new2=fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits sigma_overall=0.320 worst_q_ratio=1.254
reference average sigma_overall=0.3745 worst_q_ratio=1.2285
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278_astrometric_residuals.png (4906 matched stars from wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279_astrometric_residuals.png (4906 matched stars from wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120_astrometric_residuals.png (1537 matched stars from wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121_astrometric_residuals.png (1482 matched stars from wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits'
Saving fully-calibrated image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits'
Preparing the HTML report for the field UMa-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field UMa-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
SExtractor catalog cache: saved UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.cat to cache
SExtractor catalog cache: saved UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Creating symlink local_wcs_cache/wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.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_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits exists and is non-empty
wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits exists and is non-empty
wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits exists and is non-empty
wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits (1st reference image)
verification OK: wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Image size: 941.9'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: 12:00:03.636 +62:00:23.32 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_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits (1st new image)
verification OK: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:00:40.208 +61:59:13.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:03.636 +62:00:23.32
Second-epoch image center 12:00:40.208 +61:59:13.43
Angular distance between the image centers 0.0741 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits (2nd new image)
verification OK: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:00:37.803 +61:58:40.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:03.636 +62:00:23.32
Second-epoch image center 12:00:37.803 +61:58:40.36
Angular distance between the image centers 0.0727 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 12:00:40.208 +61:59:13.43
Second-epoch second image center 12:00:37.803 +61:58:40.36
Angular distance between the image centers 0.01032 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/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits &> /tmp/tmp.ztX64cAG7B
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits &> /tmp/tmp.c5PR7YsZCQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits &> /tmp/tmp.D9k8cCutdW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits &> /tmp/tmp.SDX7oOBIzl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.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_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.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_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
Found non-empty wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
The reference image (wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits) and catalog (wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat) found
'wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat' -> 'wcsmag.cat'
Read 37333 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.9729 to 198.6786 deg, Dec +55.2253 to +67.4860 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 159.9729 to 198.6786 deg, Dec 55.2253 to 67.4860 deg
Loaded 6642 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): 3749 out of 4194 total matches.
Matched with Tycho-2 4194 out of 37333 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.792800
a=0.000000 b=1.000000 c=22.792800
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 37333 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.9729 to 198.6786 deg, Dec +55.2253 to +67.4860 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 159.9729 to 198.6786 deg, Dec 55.2253 to 67.4860 deg
Loaded 6642 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): 3749 out of 4194 total matches.
Matched with Tycho-2 4194 out of 37333 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Forced-photometry filter: calibrated wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits -> calib.txt_param_ref_wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits (aperture=5.1)
Read 37494 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.9724 to 198.6777 deg, Dec +55.2649 to +67.4946 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 159.9724 to 198.6777 deg, Dec 55.2649 to 67.4946 deg
Loaded 6625 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): 3749 out of 4189 total matches.
Matched with Tycho-2 4189 out of 37494 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Forced-photometry filter: calibrated wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits -> calib.txt_param_ref_wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 88 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
2.1 pix UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
2.6 pix fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
2.5 pix fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Limiting magnitude estimates:
15.5 mag. UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
15.5 mag. UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
13.2 mag. fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
13.1 mag. fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.9 (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.ztX64cAG7B (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits' -> 'wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.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/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS_IMAGE_NAME=wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS-calibrated image found: wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Checking if the catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat corresponding to the image wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits alredy exist and is non-empty...
Catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat corresponding to the image wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS catalog name: wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1765, bad_region=9, passed=37315
Got 37315 stars (including 35474 good ones) from the SExtractor catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
util/solve_plate_with_UCAC5 got 37315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 4912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 4909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 37315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 4912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 37315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 37315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4909 stars left (next iteration limit 5399)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits N_match=4909 sigma_overall_arcsec=0.345 sigma_q1_arcsec=0.419 sigma_q2_arcsec=0.346 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.309 n_q1=1136 n_q2=1161 n_q3=1318 n_q4=1294 worst_quadrant_to_overall_ratio=1.215
The image catalog is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits -region wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.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.c5PR7YsZCQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits' -> 'wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.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/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS_IMAGE_NAME=wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS-calibrated image found: wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Checking if the catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat corresponding to the image wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits alredy exist and is non-empty...
Catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat corresponding to the image wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS catalog name: wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1739, bad_region=9, passed=37476
Got 37476 stars (including 35663 good ones) from the SExtractor catalog wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat
util/solve_plate_with_UCAC5 got 37476 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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 37476 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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 37476 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 37476 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4906 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits N_match=4906 sigma_overall_arcsec=0.370 sigma_q1_arcsec=0.453 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.325 n_q1=1133 n_q2=1164 n_q3=1311 n_q4=1298 worst_quadrant_to_overall_ratio=1.224
The image catalog is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits -region wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.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.D9k8cCutdW (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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
WCS_IMAGE_NAME=wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
WCS-calibrated image found: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
Checking if the catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
WCS catalog name: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=151, bad_region=10, passed=9910
Got 9910 stars (including 9735 good ones) from the SExtractor catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat
util/solve_plate_with_UCAC5 got 9910 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 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 4869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 9910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 9910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 9910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4869 stars left (next iteration limit 5355)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits N_match=4869 sigma_overall_arcsec=0.474 sigma_q1_arcsec=0.460 sigma_q2_arcsec=0.529 sigma_q3_arcsec=0.456 sigma_q4_arcsec=0.507 n_q1=1808 n_q2=917 n_q3=1413 n_q4=731 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits -region wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.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.SDX7oOBIzl (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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
WCS_IMAGE_NAME=wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
WCS-calibrated image found: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Checking if the catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
WCS catalog name: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=322, bad_region=19, passed=9792
Got 9792 stars (including 9436 good ones) from the SExtractor catalog wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
util/solve_plate_with_UCAC5 got 9792 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 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 4859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 9789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 728 to 788 (Dec 55.7 to 67.3)
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(), 9789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 9789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4860 stars left (next iteration limit 5344)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits N_match=4860 sigma_overall_arcsec=0.499 sigma_q1_arcsec=0.487 sigma_q2_arcsec=0.534 sigma_q3_arcsec=0.472 sigma_q4_arcsec=0.557 n_q1=1704 n_q2=983 n_q3=1446 n_q4=727 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits -region wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.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_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-47-11_20.00sec_-0.00C_LIGHTs_0120.fits
Saving fully-calibrated image wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.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_2026-08-05_CI_UMa-04-Q1b1x1_235835_TTUQ1b1x1_2071893_9SVjIZWM/wcs_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121.fits
Preparing the HTML report for the field UMa-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:56:49.64 +61:41:58.6: 12.84 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:51:43.96 +61:21:33.9: 12.24 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:34.58 +61:13:21.6: 12.59 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:05.95 +60:41:34.5: 13.90 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:54:44.99 +61:23:53.4: 14.03 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:36.83 +61:31:52.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:45.17 +60:51:43.4: 12.80 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:44.42 +61:16:43.9: 13.21 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:06:47.05 +61:26:17.0: 13.27 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:34.58 +61:13:21.6: 12.61 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:35.01 +61:02:21.1: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:56:49.64 +61:41:58.6: 12.86 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:51:43.96 +61:21:33.9: 12.23 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:36.83 +61:31:52.9: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter KEPT candidate at 11:55:34.58 +61:13:21.6: ref_mag=12.60 +/- 0.01 new_mean_mag=11.6219 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 11:51:43.96 +61:21:33.9: ref_mag=12.23 +/- 0.01 new_mean_mag=11.3278 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 11:56:49.64 +61:41:58.6: ref_mag=12.85 +/- 0.01 new_mean_mag=11.9258 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 13.11 +/- 0.01
Forced photometry filter KEPT candidate at 11:52:36.83 +61:31:52.9: ref_mag=13.11 +/- 0.01 new_mean_mag=12.0664 delta=1.04 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:45.17 +60:51:43.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:54:44.99 +61:23:53.4: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 11:58:45.17 +60:51:43.4: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8940 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 14.05 +/- 0.03
Forced photometry filter KEPT candidate at 11:54:44.99 +61:23:53.4: ref_mag=14.05 +/- 0.03 new_mean_mag=12.7214 delta=1.33 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:05.95 +60:41:34.5: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.03
Forced photometry filter KEPT candidate at 12:00:05.95 +60:41:34.5: ref_mag=13.93 +/- 0.03 new_mean_mag=12.7206 delta=1.21 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:44.42 +61:16:43.9: 13.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 11:59:44.42 +61:16:43.9: ref_mag=13.24 +/- 0.02 new_mean_mag=12.1900 delta=1.05 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:35.01 +61:02:21.1: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry filter KEPT candidate at 12:00:35.01 +61:02:21.1: ref_mag=13.09 +/- 0.01 new_mean_mag=12.1148 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:06:47.05 +61:26:17.0: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 12:06:47.05 +61:26:17.0: ref_mag=13.25 +/- 0.02 new_mean_mag=12.2906 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:19.49 +59:15:07.6: 13.30 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:55:18.70 +66:06:13.2: 13.36 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:19.49 +59:15:07.6: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:53:12.33 +61:35:12.0: 13.42 +/- 0.03 detection
Forced photometry filter KEPT candidate at 11:52:19.49 +59:15:07.6: ref_mag=13.31 +/- 0.02 new_mean_mag=12.3413 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:55:18.70 +66:06:13.2: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 12:55:18.70 +66:06:13.2: ref_mag=13.40 +/- 0.03 new_mean_mag=12.4734 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:53:12.33 +61:35:12.0: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 11:53:12.33 +61:35:12.0: ref_mag=13.43 +/- 0.02 new_mean_mag=12.4189 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:49:53.56 +61:07:32.2: 13.49 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:17.91 +60:23:42.6: 13.60 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:49:53.56 +61:07:32.2: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 11:49:53.56 +61:07:32.2: ref_mag=13.50 +/- 0.02 new_mean_mag=12.5071 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:17.91 +60:23:42.6: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Forced photometry filter KEPT candidate at 11:57:17.91 +60:23:42.6: ref_mag=13.62 +/- 0.02 new_mean_mag=12.5259 delta=1.09 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:03:11.87 +60:49:03.7: 13.71 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 13:08:38.85 +64:09:44.5: 13.67 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:10.57 +61:27:26.8: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 13:08:38.85 +64:09:44.5: 13.63 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:03:11.87 +60:49:03.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 13:08:38.85 +64:09:44.5: ref_mag=13.65 +/- 0.04 new_mean_mag=12.6582 delta=0.99 (need > 0.90)
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Forced photometry filter KEPT candidate at 12:03:11.87 +60:49:03.7: ref_mag=13.72 +/- 0.03 new_mean_mag=12.6039 delta=1.11 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:10.57 +61:27:26.8: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Forced photometry filter KEPT candidate at 11:55:10.57 +61:27:26.8: ref_mag=13.64 +/- 0.02 new_mean_mag=12.5690 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:16:32.45 +59:27:21.8: 13.70 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:36.94 +61:32:42.9: 13.66 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:16:32.45 +59:27:21.8: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Forced photometry filter KEPT candidate at 12:16:32.45 +59:27:21.8: ref_mag=13.72 +/- 0.03 new_mean_mag=12.7011 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:36.94 +61:32:42.9: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter KEPT candidate at 11:52:36.94 +61:32:42.9: ref_mag=13.63 +/- 0.03 new_mean_mag=12.5489 delta=1.08 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:10.92 +61:10:44.3: 13.64 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:53:41.22 +61:37:52.7: 13.64 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:10.92 +61:10:44.3: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Forced photometry filter KEPT candidate at 12:01:10.92 +61:10:44.3: ref_mag=13.63 +/- 0.02 new_mean_mag=12.6056 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:53:41.22 +61:37:52.7: 13.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Forced photometry filter KEPT candidate at 11:53:41.22 +61:37:52.7: ref_mag=13.64 +/- 0.02 new_mean_mag=12.5557 delta=1.09 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:05.14 +60:12:29.1: 13.63 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:28.79 +60:48:44.0: 13.63 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:42.25 +60:52:53.8: 13.60 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:05.14 +60:12:29.1: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.02
Forced photometry filter KEPT candidate at 11:59:05.14 +60:12:29.1: ref_mag=13.65 +/- 0.02 new_mean_mag=12.6026 delta=1.05 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:28.79 +60:48:44.0: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 12:02:28.79 +60:48:44.0: ref_mag=13.66 +/- 0.03 new_mean_mag=12.6307 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:48:59.38 +61:39:18.9: 13.61 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:42.25 +60:52:53.8: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.02
Forced photometry filter KEPT candidate at 12:00:42.25 +60:52:53.8: ref_mag=13.59 +/- 0.02 new_mean_mag=12.5024 delta=1.09 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:48:59.38 +61:39:18.9: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry filter KEPT candidate at 11:48:59.38 +61:39:18.9: ref_mag=13.61 +/- 0.02 new_mean_mag=12.5226 delta=1.09 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:03:56.13 +60:43:07.7: 13.59 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:15:16.78 +58:59:23.1: 13.60 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:03:56.13 +60:43:07.7: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 12:03:56.13 +60:43:07.7: ref_mag=13.65 +/- 0.03 new_mean_mag=12.5390 delta=1.11 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:03.00 +62:04:06.3: 13.20 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:21.35 +60:36:38.0: 13.57 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:15:16.78 +58:59:23.1: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 12:15:16.78 +58:59:23.1: ref_mag=13.59 +/- 0.03 new_mean_mag=12.6655 delta=0.92 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:03.00 +62:04:06.3: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter REJECTED candidate at 11:55:03.00 +62:04:06.3: ref_mag=13.21 +/- 0.02 new_mean_mag=12.4642 delta=0.75 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:21.35 +60:36:38.0: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter KEPT candidate at 12:01:21.35 +60:36:38.0: ref_mag=13.57 +/- 0.02 new_mean_mag=12.6099 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:43.93 +61:21:06.0: 13.57 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:43.93 +61:21:06.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 11:58:43.93 +61:21:06.0: ref_mag=13.50 +/- 0.02 new_mean_mag=12.3800 delta=1.12 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:57:14.29 +65:55:41.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:57:14.29 +65:55:41.8: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter REJECTED candidate at 12:57:14.29 +65:55:41.8: ref_mag=13.47 +/- 0.03 new_mean_mag=12.5763 delta=0.89 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:07.58 +61:41:41.8: 13.52 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:07.58 +61:41:41.8: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:54:37.54 +61:07:21.9: 13.49 +/- 0.03 detection
Forced photometry filter KEPT candidate at 11:59:07.58 +61:41:41.8: ref_mag=13.54 +/- 0.02 new_mean_mag=12.4679 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:54:37.54 +61:07:21.9: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry filter KEPT candidate at 11:54:37.54 +61:07:21.9: ref_mag=13.51 +/- 0.02 new_mean_mag=12.2868 delta=1.22 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:20.75 +61:50:48.9: 13.49 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:20.75 +61:50:48.9: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 12:02:20.75 +61:50:48.9: ref_mag=13.50 +/- 0.02 new_mean_mag=12.4186 delta=1.08 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:19:10.03 +59:58:32.3: 13.49 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:56:32.76 +61:02:09.7: 13.36 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:19:10.03 +59:58:32.3: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry filter KEPT candidate at 12:19:10.03 +59:58:32.3: ref_mag=13.47 +/- 0.02 new_mean_mag=12.4963 delta=0.97 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:56:32.76 +61:02:09.7: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter REJECTED candidate at 11:56:32.76 +61:02:09.7: ref_mag=13.39 +/- 0.02 new_mean_mag=12.5201 delta=0.87 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:06:17.19 +61:23:58.8: 13.47 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:53:59.14 +66:04:42.2: 13.45 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:06:17.19 +61:23:58.8: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 12:06:17.19 +61:23:58.8: ref_mag=13.50 +/- 0.02 new_mean_mag=12.4795 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:58.64 +61:29:47.4: 13.45 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:53:59.14 +66:04:42.2: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter KEPT candidate at 12:53:59.14 +66:04:42.2: ref_mag=13.50 +/- 0.03 new_mean_mag=12.5774 delta=0.92 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:09.39 +60:49:57.6: 13.45 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:58.64 +61:29:47.4: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 12:02:58.64 +61:29:47.4: ref_mag=13.46 +/- 0.02 new_mean_mag=12.5051 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:09.39 +60:49:57.6: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 12:02:09.39 +60:49:57.6: ref_mag=13.45 +/- 0.02 new_mean_mag=12.4385 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:54:58.09 +61:08:36.8: 13.46 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:54:58.09 +61:08:36.8: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 11:54:58.09 +61:08:36.8: ref_mag=13.46 +/- 0.02 new_mean_mag=12.2943 delta=1.17 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:51:54.89 +61:18:35.0: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:51:54.89 +61:18:35.0: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Forced photometry filter KEPT candidate at 11:51:54.89 +61:18:35.0: ref_mag=13.48 +/- 0.02 new_mean_mag=12.4610 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:48.36 +61:24:12.8: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:48.36 +61:24:12.8: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 12:01:48.36 +61:24:12.8: ref_mag=13.44 +/- 0.02 new_mean_mag=12.4546 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:32.62 +61:24:16.4: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:32.62 +61:24:16.4: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 11:57:32.62 +61:24:16.4: ref_mag=13.42 +/- 0.02 new_mean_mag=12.3790 delta=1.04 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:34.89 +61:25:21.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:34.89 +61:25:21.9: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 12:00:34.89 +61:25:21.9: ref_mag=13.39 +/- 0.02 new_mean_mag=12.4222 delta=0.97 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:44.62 +61:01:48.6: 13.38 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:44.62 +61:01:48.6: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 11:52:44.62 +61:01:48.6: ref_mag=13.40 +/- 0.02 new_mean_mag=12.3309 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:46.45 +60:41:41.4: 13.36 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:29.21 +60:51:19.3: 13.34 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:46.45 +60:41:41.4: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 11:57:46.45 +60:41:41.4: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3182 delta=1.05 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:29.21 +60:51:19.3: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 12:00:29.21 +60:51:19.3: ref_mag=13.39 +/- 0.02 new_mean_mag=12.4081 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:28.62 +61:57:44.1: 13.35 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:28.62 +61:57:44.1: 13.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 11:55:28.62 +61:57:44.1: ref_mag=13.35 +/- 0.02 new_mean_mag=12.3985 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:02.31 +61:10:14.4: 13.34 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:02.31 +61:10:14.4: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 12:01:02.31 +61:10:14.4: ref_mag=13.36 +/- 0.02 new_mean_mag=12.3724 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:13.87 +61:37:05.8: 13.31 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:13.87 +61:37:05.8: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 11:55:13.87 +61:37:05.8: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3098 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:50.61 +61:00:37.1: 13.31 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:50.61 +61:00:37.1: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 12:01:50.61 +61:00:37.1: ref_mag=13.33 +/- 0.02 new_mean_mag=12.2945 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:03.34 +61:30:44.9: 13.30 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:03.34 +61:30:44.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 11:59:03.34 +61:30:44.9: ref_mag=13.32 +/- 0.02 new_mean_mag=12.3843 delta=0.94 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:49:38.18 +60:59:54.9: 13.27 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:49:38.18 +60:59:54.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 11:49:38.18 +60:59:54.9: ref_mag=13.24 +/- 0.02 new_mean_mag=12.2795 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:02:34.21 +62:05:01.9: 13.19 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:02:34.21 +62:05:01.9: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.01
Forced photometry filter KEPT candidate at 12:02:34.21 +62:05:01.9: ref_mag=13.19 +/- 0.01 new_mean_mag=12.1926 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:50:58.06 +61:23:41.4: 13.18 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:50:58.06 +61:23:41.4: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 11:50:58.06 +61:23:41.4: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1272 delta=1.04 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:44.41 +61:35:58.0: 13.16 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:23.19 +61:19:57.2: 13.16 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:44.41 +61:35:58.0: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Forced photometry filter KEPT candidate at 11:58:44.41 +61:35:58.0: ref_mag=13.15 +/- 0.01 new_mean_mag=12.2324 delta=0.92 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:23.19 +61:19:57.2: 13.14 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:49:22.81 +61:33:39.9: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Forced photometry filter KEPT candidate at 11:57:23.19 +61:19:57.2: ref_mag=13.15 +/- 0.01 new_mean_mag=12.0904 delta=1.06 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:49:22.81 +61:33:39.9: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Forced photometry filter KEPT candidate at 11:49:22.81 +61:33:39.9: ref_mag=13.15 +/- 0.01 new_mean_mag=12.2082 delta=0.94 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:59:15.68 +61:17:13.9: 13.13 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:59:15.68 +61:17:13.9: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 11:59:15.68 +61:17:13.9: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1734 delta=0.97 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:58.80 +60:47:59.6: 13.13 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:58.80 +60:47:59.6: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.01
Forced photometry filter KEPT candidate at 11:55:58.80 +60:47:59.6: ref_mag=13.13 +/- 0.01 new_mean_mag=12.1327 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:25:07.83 +60:25:14.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:25:07.83 +60:25:14.3: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter REJECTED candidate at 12:25:07.83 +60:25:14.3: ref_mag=12.92 +/- 0.01 new_mean_mag=12.1900 delta=0.73 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:00.91 +61:00:01.3: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:49:00.81 +61:00:55.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:00.91 +61:00:01.3: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry filter KEPT candidate at 11:57:00.91 +61:00:01.3: ref_mag=13.09 +/- 0.01 new_mean_mag=12.0213 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:44.15 +61:24:53.3: 12.88 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:49:00.81 +61:00:55.1: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.01
Forced photometry filter KEPT candidate at 11:49:00.81 +61:00:55.1: ref_mag=13.04 +/- 0.01 new_mean_mag=12.1104 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:44.15 +61:24:53.3: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 12:00:44.15 +61:24:53.3: ref_mag=12.89 +/- 0.01 new_mean_mag=11.9865 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:22.27 +61:27:51.9: 12.87 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:22.27 +61:27:51.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 11:55:22.27 +61:27:51.9: ref_mag=12.90 +/- 0.01 new_mean_mag=11.8724 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:09.20 +61:20:51.6: 12.86 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:09.20 +61:20:51.6: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 11:55:09.20 +61:20:51.6: ref_mag=12.88 +/- 0.01 new_mean_mag=11.8839 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:13.08 +61:06:51.8: 12.77 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:53:18.65 +61:20:18.0: 12.69 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:01:09.64 +61:41:15.9: 12.48 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:13.08 +61:06:51.8: 12.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 11:58:13.08 +61:06:51.8: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7796 delta=0.97 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:53:18.65 +61:20:18.0: 12.73 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:01:09.64 +61:41:15.9: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter REJECTED candidate at 11:53:18.65 +61:20:18.0: ref_mag=12.71 +/- 0.01 new_mean_mag=11.8112 delta=0.89 (need > 0.90)
Forced photometry filter KEPT candidate at 12:01:09.64 +61:41:15.9: ref_mag=12.47 +/- 0.01 new_mean_mag=11.5426 delta=0.92 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:55:03.10 +60:57:56.1: 14.23 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:55:03.10 +60:57:56.1: 14.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.04
Forced photometry filter KEPT candidate at 11:55:03.10 +60:57:56.1: ref_mag=14.28 +/- 0.04 new_mean_mag=12.9401 delta=1.34 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:53:06.22 +61:16:03.2: 14.01 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:53:06.22 +61:16:03.2: 14.00 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.03
Forced photometry filter KEPT candidate at 11:53:06.22 +61:16:03.2: ref_mag=14.00 +/- 0.03 new_mean_mag=12.6924 delta=1.31 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:56:16.14 +61:22:43.6: 14.01 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:56:16.14 +61:22:43.6: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.03
Forced photometry filter KEPT candidate at 11:56:16.14 +61:22:43.6: ref_mag=14.01 +/- 0.03 new_mean_mag=12.7699 delta=1.24 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:56:11.42 +61:21:11.9: 13.90 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:29.74 +60:21:33.9: 13.96 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:29.74 +60:21:33.9: 13.99 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:56:11.42 +61:21:11.9: 13.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.03
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Forced photometry filter KEPT candidate at 12:00:29.74 +60:21:33.9: ref_mag=13.97 +/- 0.03 new_mean_mag=12.7541 delta=1.22 (need > 0.90)
Forced photometry filter KEPT candidate at 11:56:11.42 +61:21:11.9: ref_mag=13.91 +/- 0.03 new_mean_mag=12.6784 delta=1.23 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:57:05.68 +61:09:39.4: 13.81 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:57:05.68 +61:09:39.4: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 11:57:05.68 +61:09:39.4: ref_mag=13.81 +/- 0.03 new_mean_mag=12.6512 delta=1.16 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:00:48.84 +61:00:46.9: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:00:48.84 +61:00:46.9: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 12:00:48.84 +61:00:46.9: ref_mag=13.81 +/- 0.03 new_mean_mag=12.7018 delta=1.11 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:20:36.17 +60:10:14.3: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:20:36.17 +60:10:14.3: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry filter KEPT candidate at 12:20:36.17 +60:10:14.3: ref_mag=13.78 +/- 0.03 new_mean_mag=12.7247 delta=1.05 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:58:54.38 +60:59:32.4: 13.75 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:58:54.38 +60:59:32.4: 13.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 11:58:54.38 +60:59:32.4: ref_mag=13.71 +/- 0.03 new_mean_mag=12.5844 delta=1.13 (need > 0.90)
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:52:17.28 +61:49:49.9: 13.72 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q1b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:52:17.28 +61:49:49.9: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 11:52:17.28 +61:49:49.9: ref_mag=13.77 +/- 0.03 new_mean_mag=12.5899 delta=1.18 (need > 0.90)
Adding exclusion_list_local.txt__out06672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34719.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 110s
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: 40s
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Considering the candidate 52846_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 52846_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 12:15:42.38 +57:00:10.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 53186_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 53186_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 12:15:28.56 +56:59:06.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 53250_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 53250_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 11:58:21.18 +61:26:10.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 12953_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 12953_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15729_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15729_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15714_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15714_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15036_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15036_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 13649_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 13649_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 16686_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16686_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 16337_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16337_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14128_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14128_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15039_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15039_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15292_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15292_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 08502_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 08502_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 25477_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 25477_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 16521_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16521_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15077_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15077_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 12121_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 12121_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 13270_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 13270_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 34719_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 34719_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15928_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15928_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 08173_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 08173_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 16429_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16429_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14563_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14563_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 16636_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16636_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 36279_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 36279_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 13:03:41.52 +63:43:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11406_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 11406_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 13278_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 13278_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 13630_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 13630_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 17030_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 17030_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 12885_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 12885_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 06672_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 06672_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 18082_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 18082_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
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Considering the candidate 12632_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 12632_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15372_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15372_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 29658_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 29658_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
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Considering the candidate 16575_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16575_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14757_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14757_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 16947_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16947_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 09873_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 09873_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14333_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 14333_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
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Considering the candidate 15184_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15184_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 29202_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 29202_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15634_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15634_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 13377_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 13377_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14808_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14808_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15580_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15580_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15391_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15391_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15593_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15593_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15499_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15499_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14508_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14508_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 13080_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 13080_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 13537_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 13537_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 17669_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 17669_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14546_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14546_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 16512_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16512_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 13951_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 13951_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15896_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15896_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14594_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14594_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 17708_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 17708_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15959_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15959_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 16212_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16212_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15361_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15361_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 16665_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16665_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15087_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15087_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 13589_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 13589_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 11320_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 11320_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
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Considering the candidate 14165_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14165_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14700_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14700_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15460_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15460_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15929_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15929_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15512_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15512_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14492_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14492_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15486_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 15486_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
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Considering the candidate 16393_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 16393_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14183_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14183_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15402_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15402_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15582_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15582_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 11853_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 11853_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 15516_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 15516_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 26862_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 26862_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 11:58:43.26 +63:21:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07651_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 07651_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 12:36:23.35 +59:29:13.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14746_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14746_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14025_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14025_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 10506_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 10506_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 14047_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 14047_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 17369_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 17369_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21303_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121
The candidate 21303_fd_UMa-04-Q1b1x1_2026-08-05_23-48-42_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 11:03:43.67 +61:45:03.5 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 157s
Prepared the HTML report for the field UMa-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
12:15:16.78 +58:59:23.1
12:16:32.45 +59:27:21.8
11:52:19.49 +59:15:07.6
12:19:10.03 +59:58:32.3
12:20:36.17 +60:10:14.3
11:59:05.14 +60:12:29.1
12:00:29.74 +60:21:33.9
11:57:17.91 +60:23:42.6
12:01:21.35 +60:36:38.0
12:03:56.13 +60:43:07.7
12:00:05.95 +60:41:34.5
11:57:46.45 +60:41:41.4
12:03:11.87 +60:49:03.7
12:02:28.79 +60:48:44.0
12:02:09.39 +60:49:57.6
12:00:29.21 +60:51:19.3
11:55:58.80 +60:47:59.6
12:00:42.25 +60:52:53.8
11:58:45.17 +60:51:43.4
12:01:50.61 +61:00:37.1
12:00:48.84 +61:00:46.9
11:58:54.38 +60:59:32.4
12:00:35.01 +61:02:21.1
11:57:00.91 +61:00:01.3
11:55:03.10 +60:57:56.1
11:58:13.08 +61:06:51.8
11:52:44.62 +61:01:48.6
12:01:02.31 +61:10:14.4
12:01:10.92 +61:10:44.3
11:49:38.18 +60:59:54.9
11:49:00.81 +61:00:55.1
11:57:05.68 +61:09:39.4
11:54:37.54 +61:07:21.9
11:54:58.09 +61:08:36.8
11:55:34.58 +61:13:21.6
11:59:44.42 +61:16:43.9
11:49:53.56 +61:07:32.2
11:59:15.68 +61:17:13.9
12:06:17.19 +61:23:58.8
12:06:47.05 +61:26:17.0
11:57:23.19 +61:19:57.2
11:58:43.93 +61:21:06.0
12:01:48.36 +61:24:12.8
11:53:06.22 +61:16:03.2
12:00:44.15 +61:24:53.3
12:00:34.89 +61:25:21.9
11:55:09.20 +61:20:51.6
11:56:11.42 +61:21:11.9
11:51:54.89 +61:18:35.0
11:56:16.14 +61:22:43.6
11:57:32.62 +61:24:16.4
12:02:58.64 +61:29:47.4
11:51:43.96 +61:21:33.9
11:54:44.99 +61:23:53.4
11:59:03.34 +61:30:44.9
11:55:10.57 +61:27:26.8
11:55:22.27 +61:27:51.9
11:50:58.06 +61:23:41.4
11:58:44.41 +61:35:58.0
11:52:36.83 +61:31:52.9
12:01:09.64 +61:41:15.9
11:52:36.94 +61:32:42.9
11:55:13.87 +61:37:05.8
11:53:12.33 +61:35:12.0
11:59:07.58 +61:41:41.8
11:53:41.22 +61:37:52.7
11:49:22.81 +61:33:39.9
11:56:49.64 +61:41:58.6
12:02:20.75 +61:50:48.9
11:48:59.38 +61:39:18.9
11:52:17.28 +61:49:49.9
11:55:28.62 +61:57:44.1
12:02:34.21 +62:05:01.9
12:55:18.70 +66:06:13.2
12:53:59.14 +66:04:42.2
13:08:38.85 +64:09:44.5
########### Completed UMa-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
12:00:05.95 +60:41:34.5
11:54:44.99 +61:23:53.4
11:51:43.96 +61:21:33.9
11:55:34.58 +61:13:21.6
11:58:45.17 +60:51:43.4
11:56:49.64 +61:41:58.6
11:52:36.83 +61:31:52.9
12:00:35.01 +61:02:21.1
11:59:44.42 +61:16:43.9
12:06:47.05 +61:26:17.0
11:52:19.49 +59:15:07.6
12:55:18.70 +66:06:13.2
11:53:12.33 +61:35:12.0
11:49:53.56 +61:07:32.2
11:57:17.91 +60:23:42.6
12:03:11.87 +60:49:03.7
13:08:38.85 +64:09:44.5
11:55:10.57 +61:27:26.8
12:16:32.45 +59:27:21.8
11:52:36.94 +61:32:42.9
12:01:10.92 +61:10:44.3
11:53:41.22 +61:37:52.7
11:59:05.14 +60:12:29.1
12:02:28.79 +60:48:44.0
12:00:42.25 +60:52:53.8
11:48:59.38 +61:39:18.9
12:03:56.13 +60:43:07.7
12:15:16.78 +58:59:23.1
12:01:21.35 +60:36:38.0
11:58:43.93 +61:21:06.0
11:59:07.58 +61:41:41.8
11:54:37.54 +61:07:21.9
12:02:20.75 +61:50:48.9
12:19:10.03 +59:58:32.3
12:06:17.19 +61:23:58.8
12:53:59.14 +66:04:42.2
12:02:58.64 +61:29:47.4
12:02:09.39 +60:49:57.6
11:54:58.09 +61:08:36.8
11:51:54.89 +61:18:35.0
12:01:48.36 +61:24:12.8
11:57:32.62 +61:24:16.4
12:00:34.89 +61:25:21.9
11:52:44.62 +61:01:48.6
11:57:46.45 +60:41:41.4
12:00:29.21 +60:51:19.3
11:55:28.62 +61:57:44.1
12:01:02.31 +61:10:14.4
11:55:13.87 +61:37:05.8
12:01:50.61 +61:00:37.1
11:59:03.34 +61:30:44.9
11:49:38.18 +60:59:54.9
12:02:34.21 +62:05:01.9
11:50:58.06 +61:23:41.4
11:58:44.41 +61:35:58.0
11:57:23.19 +61:19:57.2
11:49:22.81 +61:33:39.9
11:59:15.68 +61:17:13.9
11:55:58.80 +60:47:59.6
11:57:00.91 +61:00:01.3
11:49:00.81 +61:00:55.1
12:00:44.15 +61:24:53.3
11:55:22.27 +61:27:51.9
11:55:09.20 +61:20:51.6
11:58:13.08 +61:06:51.8
12:01:09.64 +61:41:15.9
11:55:03.10 +60:57:56.1
11:53:06.22 +61:16:03.2
11:56:16.14 +61:22:43.6
12:00:29.74 +60:21:33.9
11:56:11.42 +61:21:11.9
11:57:05.68 +61:09:39.4
12:00:48.84 +61:00:46.9
12:20:36.17 +60:10:14.3
11:58:54.38 +60:59:32.4
11:52:17.28 +61:49:49.9
###################################################################################
12:00:05.95 +60:41:34.5 -- not an asteroid (will add it to exclusion list)
11:54:44.99 +61:23:53.4 -- not an asteroid (will add it to exclusion list)
11:51:43.96 +61:21:33.9 -- not an asteroid (will add it to exclusion list)
11:55:34.58 +61:13:21.6 -- not an asteroid (will add it to exclusion list)
11:58:45.17 +60:51:43.4 -- not an asteroid (will add it to exclusion list)
11:56:49.64 +61:41:58.6 -- not an asteroid (will add it to exclusion list)
11:52:36.83 +61:31:52.9 -- not an asteroid (will add it to exclusion list)
12:00:35.01 +61:02:21.1 -- not an asteroid (will add it to exclusion list)
11:59:44.42 +61:16:43.9 -- not an asteroid (will add it to exclusion list)
12:06:47.05 +61:26:17.0 -- not an asteroid (will add it to exclusion list)
11:52:19.49 +59:15:07.6 -- not an asteroid (will add it to exclusion list)
12:55:18.70 +66:06:13.2 -- not an asteroid (will add it to exclusion list)
11:53:12.33 +61:35:12.0 -- not an asteroid (will add it to exclusion list)
11:49:53.56 +61:07:32.2 -- not an asteroid (will add it to exclusion list)
11:57:17.91 +60:23:42.6 -- not an asteroid (will add it to exclusion list)
12:03:11.87 +60:49:03.7 -- not an asteroid (will add it to exclusion list)
13:08:38.85 +64:09:44.5 -- not an asteroid (will add it to exclusion list)
11:55:10.57 +61:27:26.8 -- not an asteroid (will add it to exclusion list)
12:16:32.45 +59:27:21.8 -- not an asteroid (will add it to exclusion list)
11:52:36.94 +61:32:42.9 -- not an asteroid (will add it to exclusion list)
12:01:10.92 +61:10:44.3 -- not an asteroid (will add it to exclusion list)
11:53:41.22 +61:37:52.7 -- not an asteroid (will add it to exclusion list)
11:59:05.14 +60:12:29.1 -- not an asteroid (will add it to exclusion list)
12:02:28.79 +60:48:44.0 -- not an asteroid (will add it to exclusion list)
12:00:42.25 +60:52:53.8 -- not an asteroid (will add it to exclusion list)
11:48:59.38 +61:39:18.9 -- not an asteroid (will add it to exclusion list)
12:03:56.13 +60:43:07.7 -- not an asteroid (will add it to exclusion list)
12:15:16.78 +58:59:23.1 -- not an asteroid (will add it to exclusion list)
12:01:21.35 +60:36:38.0 -- not an asteroid (will add it to exclusion list)
11:58:43.93 +61:21:06.0 -- not an asteroid (will add it to exclusion list)
11:59:07.58 +61:41:41.8 -- not an asteroid (will add it to exclusion list)
11:54:37.54 +61:07:21.9 -- not an asteroid (will add it to exclusion list)
12:02:20.75 +61:50:48.9 -- not an asteroid (will add it to exclusion list)
12:19:10.03 +59:58:32.3 -- not an asteroid (will add it to exclusion list)
12:06:17.19 +61:23:58.8 -- not an asteroid (will add it to exclusion list)
12:53:59.14 +66:04:42.2 -- not an asteroid (will add it to exclusion list)
12:02:58.64 +61:29:47.4 -- not an asteroid (will add it to exclusion list)
12:02:09.39 +60:49:57.6 -- not an asteroid (will add it to exclusion list)
11:54:58.09 +61:08:36.8 -- not an asteroid (will add it to exclusion list)
11:51:54.89 +61:18:35.0 -- not an asteroid (will add it to exclusion list)
12:01:48.36 +61:24:12.8 -- not an asteroid (will add it to exclusion list)
11:57:32.62 +61:24:16.4 -- not an asteroid (will add it to exclusion list)
12:00:34.89 +61:25:21.9 -- not an asteroid (will add it to exclusion list)
11:52:44.62 +61:01:48.6 -- not an asteroid (will add it to exclusion list)
11:57:46.45 +60:41:41.4 -- not an asteroid (will add it to exclusion list)
12:00:29.21 +60:51:19.3 -- not an asteroid (will add it to exclusion list)
11:55:28.62 +61:57:44.1 -- not an asteroid (will add it to exclusion list)
12:01:02.31 +61:10:14.4 -- not an asteroid (will add it to exclusion list)
11:55:13.87 +61:37:05.8 -- not an asteroid (will add it to exclusion list)
12:01:50.61 +61:00:37.1 -- not an asteroid (will add it to exclusion list)
11:59:03.34 +61:30:44.9 -- not an asteroid (will add it to exclusion list)
11:49:38.18 +60:59:54.9 -- not an asteroid (will add it to exclusion list)
12:02:34.21 +62:05:01.9 -- not an asteroid (will add it to exclusion list)
11:50:58.06 +61:23:41.4 -- not an asteroid (will add it to exclusion list)
11:58:44.41 +61:35:58.0 -- not an asteroid (will add it to exclusion list)
11:57:23.19 +61:19:57.2 -- not an asteroid (will add it to exclusion list)
11:49:22.81 +61:33:39.9 -- not an asteroid (will add it to exclusion list)
11:59:15.68 +61:17:13.9 -- not an asteroid (will add it to exclusion list)
11:55:58.80 +60:47:59.6 -- not an asteroid (will add it to exclusion list)
11:57:00.91 +61:00:01.3 -- not an asteroid (will add it to exclusion list)
11:49:00.81 +61:00:55.1 -- not an asteroid (will add it to exclusion list)
12:00:44.15 +61:24:53.3 -- not an asteroid (will add it to exclusion list)
11:55:22.27 +61:27:51.9 -- not an asteroid (will add it to exclusion list)
11:55:09.20 +61:20:51.6 -- not an asteroid (will add it to exclusion list)
11:58:13.08 +61:06:51.8 -- not an asteroid (will add it to exclusion list)
12:01:09.64 +61:41:15.9 -- not an asteroid (will add it to exclusion list)
11:55:03.10 +60:57:56.1 -- not an asteroid (will add it to exclusion list)
11:53:06.22 +61:16:03.2 -- not an asteroid (will add it to exclusion list)
11:56:16.14 +61:22:43.6 -- not an asteroid (will add it to exclusion list)
12:00:29.74 +60:21:33.9 -- not an asteroid (will add it to exclusion list)
11:56:11.42 +61:21:11.9 -- not an asteroid (will add it to exclusion list)
11:57:05.68 +61:09:39.4 -- not an asteroid (will add it to exclusion list)
12:00:48.84 +61:00:46.9 -- not an asteroid (will add it to exclusion list)
12:20:36.17 +60:10:14.3 -- not an asteroid (will add it to exclusion list)
11:58:54.38 +60:59:32.4 -- not an asteroid (will add it to exclusion list)
11:52:17.28 +61:49:49.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
11:48:59.38 +61:39:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:49:00.81 +61:00:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:49:22.81 +61:33:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:49:38.18 +60:59:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:49:53.56 +61:07:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:50:58.06 +61:23:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:51:43.96 +61:21:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:51:54.89 +61:18:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:52:17.28 +61:49:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:52:19.49 +59:15:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:52:36.83 +61:31:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:52:36.94 +61:32:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:52:44.62 +61:01:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:53:06.22 +61:16:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:53:12.33 +61:35:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:53:41.22 +61:37:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:54:37.54 +61:07:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:54:44.99 +61:23:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:54:58.09 +61:08:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:03.10 +60:57:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:09.20 +61:20:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:10.57 +61:27:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:13.87 +61:37:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:22.27 +61:27:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:28.62 +61:57:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:34.58 +61:13:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:58.80 +60:47:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:56:11.42 +61:21:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:56:16.14 +61:22:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:56:49.64 +61:41:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:57:00.91 +61:00:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:57:05.68 +61:09:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:57:17.91 +60:23:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:57:23.19 +61:19:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:57:32.62 +61:24:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:57:46.45 +60:41:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:58:13.08 +61:06:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:58:43.93 +61:21:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:58:44.41 +61:35:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:58:45.17 +60:51:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:58:54.38 +60:59:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:59:03.34 +61:30:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:59:05.14 +60:12:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:59:07.58 +61:41:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:59:15.68 +61:17:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:59:44.42 +61:16:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:00:05.95 +60:41:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:00:29.21 +60:51:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:00:29.74 +60:21:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:00:34.89 +61:25:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:00:35.01 +61:02:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:00:42.25 +60:52:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:00:44.15 +61:24:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:00:48.84 +61:00:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:01:02.31 +61:10:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:01:09.64 +61:41:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:01:10.92 +61:10:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:01:21.35 +60:36:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:01:48.36 +61:24:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:01:50.61 +61:00:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:02:09.39 +60:49:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:02:20.75 +61:50:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:02:28.79 +60:48:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:02:34.21 +62:05:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:02:58.64 +61:29:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:03:11.87 +60:49:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:03:56.13 +60:43:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:06:17.19 +61:23:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:06:47.05 +61:26:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:15:16.78 +58:59:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:16:32.45 +59:27:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:19:10.03 +59:58:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:20:36.17 +60:10:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:59.14 +66:04:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:18.70 +66:06:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:08:38.85 +64:09:44.5 -- 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)
11:48:59.38 +61:39:18.9 -- a known variable star
11:49:00.81 +61:00:55.1 -- not a known variable star
11:49:22.81 +61:33:39.9 -- not a known variable star
11:49:38.18 +60:59:54.9 -- not a known variable star
11:49:53.56 +61:07:32.2 -- not a known variable star
11:50:58.06 +61:23:41.4 -- not a known variable star
11:51:43.96 +61:21:33.9 -- not a known variable star
11:51:54.89 +61:18:35.0 -- not a known variable star
11:52:17.28 +61:49:49.9 -- not a known variable star
11:52:19.49 +59:15:07.6 -- not a known variable star
11:52:36.83 +61:31:52.9 -- not a known variable star
11:52:36.94 +61:32:42.9 -- not a known variable star
11:52:44.62 +61:01:48.6 -- not a known variable star
11:53:06.22 +61:16:03.2 -- not a known variable star
11:53:12.33 +61:35:12.0 -- not a known variable star
11:53:41.22 +61:37:52.7 -- not a known variable star
11:54:37.54 +61:07:21.9 -- not a known variable star
11:54:44.99 +61:23:53.4 -- not a known variable star
11:54:58.09 +61:08:36.8 -- not a known variable star
11:55:03.10 +60:57:56.1 -- not a known variable star
11:55:09.20 +61:20:51.6 -- not a known variable star
11:55:10.57 +61:27:26.8 -- not a known variable star
11:55:13.87 +61:37:05.8 -- not a known variable star
11:55:22.27 +61:27:51.9 -- not a known variable star
11:55:28.62 +61:57:44.1 -- not a known variable star
11:55:34.58 +61:13:21.6 -- not a known variable star
11:55:58.80 +60:47:59.6 -- not a known variable star
11:56:11.42 +61:21:11.9 -- not a known variable star
11:56:16.14 +61:22:43.6 -- not a known variable star
11:56:49.64 +61:41:58.6 -- not a known variable star
11:57:00.91 +61:00:01.3 -- not a known variable star
11:57:05.68 +61:09:39.4 -- not a known variable star
11:57:17.91 +60:23:42.6 -- not a known variable star
11:57:23.19 +61:19:57.2 -- not a known variable star
11:57:32.62 +61:24:16.4 -- not a known variable star
11:57:46.45 +60:41:41.4 -- not a known variable star
11:58:13.08 +61:06:51.8 -- not a known variable star
11:58:43.93 +61:21:06.0 -- not a known variable star
11:58:44.41 +61:35:58.0 -- not a known variable star
11:58:45.17 +60:51:43.4 -- not a known variable star
11:58:54.38 +60:59:32.4 -- not a known variable star
11:59:03.34 +61:30:44.9 -- not a known variable star
11:59:05.14 +60:12:29.1 -- not a known variable star
11:59:07.58 +61:41:41.8 -- not a known variable star
11:59:15.68 +61:17:13.9 -- not a known variable star
11:59:44.42 +61:16:43.9 -- not a known variable star
12:00:05.95 +60:41:34.5 -- not a known variable star
12:00:29.21 +60:51:19.3 -- not a known variable star
12:00:29.74 +60:21:33.9 -- a known variable star
12:00:34.89 +61:25:21.9 -- not a known variable star
12:00:35.01 +61:02:21.1 -- not a known variable star
12:00:42.25 +60:52:53.8 -- not a known variable star
12:00:44.15 +61:24:53.3 -- not a known variable star
12:00:48.84 +61:00:46.9 -- not a known variable star
12:01:02.31 +61:10:14.4 -- not a known variable star
12:01:09.64 +61:41:15.9 -- not a known variable star
12:01:10.92 +61:10:44.3 -- not a known variable star
12:01:21.35 +60:36:38.0 -- not a known variable star
12:01:48.36 +61:24:12.8 -- not a known variable star
12:01:50.61 +61:00:37.1 -- not a known variable star
12:02:09.39 +60:49:57.6 -- not a known variable star
12:02:20.75 +61:50:48.9 -- not a known variable star
12:02:28.79 +60:48:44.0 -- not a known variable star
12:02:34.21 +62:05:01.9 -- not a known variable star
12:02:58.64 +61:29:47.4 -- not a known variable star
12:03:11.87 +60:49:03.7 -- not a known variable star
12:03:56.13 +60:43:07.7 -- not a known variable star
12:06:17.19 +61:23:58.8 -- not a known variable star
12:06:47.05 +61:26:17.0 -- not a known variable star
12:15:16.78 +58:59:23.1 -- a known variable star
12:16:32.45 +59:27:21.8 -- not a known variable star
12:19:10.03 +59:58:32.3 -- not a known variable star
12:20:36.17 +60:10:14.3 -- not a known variable star
12:53:59.14 +66:04:42.2 -- not a known variable star
12:55:18.70 +66:06:13.2 -- not a known variable star
13:08:38.85 +64:09:44.5 -- not a known variable star
Found 73 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
76 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 76 (excluding asteroids and hot pixels, 73 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)2461258.69955678 -observatory V36
07:45:31.03 +20:23:14.0 Mercury (-0.3mag)
11:55:36.81 -00:03:25.1 Venus (-4.3mag)
05:43:22.86 +23:32:37.2 Mars (1.3mag)
08:41:07.04 +18:48:02.2 Jupiter (-1.8mag)
00:56:33.04 +03:16:47.8 Saturn (0.6mag)
04:11:29.56 +20:56:20.2 Uranus (5.8mag)
00:16:12.86 +00:13:59.3 Neptune (7.7mag)
20:28:20.12 -23:29:23.8 Pluto (14.4mag)
02:45:39.21 +20:28:22.5 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 00:01 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461258.69955678:
08:41:14.14 +18:47:32.0 Io (6.0mag)
08:41:04.08 +18:48:15.3 Europa (6.3mag)
08:41:03.31 +18:48:22.1 Ganymede (5.6mag)
08:40:53.12 +18:49:04.7 Callisto (6.7mag)
08:38:42.94 +18:46:11.3 Himalia (15.7mag)
08:41:05.46 +18:48:09.8 Thebe (16.6mag)
08:38:13.57 +18:45:06.9 Elara (17.7mag)
08:45:12.93 +18:28:27.4 Pasiphae (17.9mag)
08:44:25.93 +18:57:52.3 Carme (19.0mag)
00:56:30.90 +03:17:14.7 Titan (8.4mag)
00:56:27.36 +03:16:51.9 Rhea (9.7mag)
00:56:36.62 +03:15:09.8 Iapetus (11.1mag)
00:56:19.67 +03:17:02.3 Hyperion (14.4mag)
00:55:58.10 +03:10:14.7 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 00:01 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.69955678:
18:55:37.83 -24:04:09.9 JWST
17:12:50.08 +42:16:20.1 Chandra
09:16:49.55 -52:23:53.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 00:01 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.69955678 -observatory V36
03:11:21.81 +17:12:20.2 17.7mag P/1996 R2 (Lagerkvist)
18:02:25.00 -34:38:24.3 14.0mag P/2010 H2 (Vales)
06:51:53.78 -68:49:36.7 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:16.68 +32:57:03.6 17.7mag C/2017 K2 (PANSTARRS)
03:37:39.00 +36:43:15.0 16.7mag P/2021 N1 (ZTF)
22:40:17.80 +31:34:00.4 17.3mag C/2022 E2 (ATLAS)
06:41:27.55 +26:34:32.8 16.8mag C/2022 N2 (PANSTARRS)
10:19:41.74 +28:33:38.7 17.0mag C/2022 QE78 (ATLAS)
09:27:30.18 +05:17:43.1 17.9mag C/2022 R6 (PANSTARRS)
15:12:08.99 -12:12:25.6 17.9mag P/2023 B1 (PANSTARRS)
21:13:26.87 +66:14:03.0 17.9mag C/2023 H5 (Lemmon)
15:49:55.75 -12:44:49.0 14.3mag C/2023 R1 (PANSTARRS)
08:05:48.64 +31:15:17.1 15.2mag C/2024 E1 (Wierzchos)
15:07:18.02 +15:36:58.9 17.7mag C/2024 G6 (ATLAS)
19:05:42.15 +42:57:36.8 13.7mag C/2024 J3 (ATLAS)
21:13:42.09 +49:04:37.0 17.6mag C/2024 R4 (PANSTARRS)
05:13:30.24 -12:59:39.4 15.5mag C/2024 T5 (ATLAS)
06:54:53.97 +24:30:43.2 17.9mag C/2025 J1 (Borisov)
07:29:56.28 -15:51:49.8 17.7mag C/2025 R3 (PANSTARRS)
10:30:05.62 +21:01:57.4 17.3mag C/2025 V2 (Rankin)
12:56:55.61 +02:29:00.9 17.0mag C/2025 Y1 (ATLAS)
16:03:42.74 +78:01:14.5 16.8mag C/2026 A2 (Bok)
03:06:42.41 +46:08:40.8 17.1mag C/2026 B2 (Sun-Gao)
11:45:07.68 +08:19:47.9 17.3mag A/2026 E1
21:56:05.49 -26:26:45.5 6.9mag 10P/Tempel
11:27:45.17 -03:16:30.1 16.2mag 29P/Schwassmann-Wachmann
04:36:43.60 +32:15:35.3 18.0mag 47P/Ashbrook-Jackson
11:03:33.55 +05:18:16.2 17.2mag 63P/Wild
00:54:17.95 -05:22:39.8 15.4mag 65P/Gunn
05:30:56.74 +20:43:47.4 13.7mag 78P/Gehrels
20:39:48.88 -23:17:21.5 17.8mag 84P/Giclas
02:58:41.96 +13:32:15.8 16.7mag 88P/Howell
07:50:41.97 +27:55:53.9 16.1mag 93P/Lovas
04:00:39.85 +16:05:13.7 17.6mag 112P/Urata-Niijima
05:49:47.24 +30:31:01.0 16.3mag 114P/Wiseman-Skiff
09:13:41.34 +26:59:24.2 15.0mag 123P/West-Hartley
11:39:41.13 -09:29:20.4 17.1mag 124P/Mrkos
05:33:33.64 +21:11:10.6 16.1mag 128P/Shoemaker-Holt
06:25:02.50 +18:59:50.1 17.9mag 131P/Mueller
00:03:42.04 +03:25:22.1 17.6mag 139P/Vaisala-Oterma
03:21:34.41 -19:44:57.3 14.0mag 161P/Hartley-IRAS
07:09:09.19 +37:41:17.7 15.8mag 162P/SidingSpring
15:50:21.46 +39:28:23.3 12.3mag 169P/NEAT
02:39:15.61 +09:28:29.5 17.6mag 220P/McNaught
16:40:34.66 -09:56:33.9 17.6mag 235P/LINEAR
20:23:45.14 -52:50:55.2 17.8mag 259P/Garradd
03:16:12.78 +24:18:32.8 15.4mag 260P/McNaught
06:59:15.71 +37:45:18.3 17.3mag 295P/LINEAR
15:09:50.55 +03:21:41.7 17.7mag 391P/Kowalski
08:59:02.32 +18:28:30.8 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 00:01 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
-rw-r--r-- 1 apache apache 5.7K Aug 6 00:01 asassn_transients_list.txt
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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 00:01 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
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
18:14:11.533 +25:31:50.45 AT 2026vkg 2026-07-16.29 20.95
22:50:03.729 +40:38:42.44 AT 2026vkf 2026-07-20.53 20.32
-rw-r--r-- 1 apache apache 87K Aug 6 00:01 tns_transients_list.txt
