This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg
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 07 17.2373 2461238.7374 13.02 12:37:37.50 +66:04:05.6
125.15704 51.00031 galactic Dra Second-epoch detections are separated by 1.2" 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 | 12:37:37.50 +66:04:05.6 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:37:37.50 +66:04:05.6: 13.98 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:37:37.50 +66:04:05.6: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461238.7374,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.51 11:26:26.33 +58:31:59.6
142.33102 55.27732 galactic UMa Second-epoch detections are separated by 1.3" and 7.0 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 | 11:26:26.33 +58:31:59.6 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:26:26.33 +58:31:59.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:26:26.33 +58:31:59.6: 13.54 +/- 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 07 17.2373* 11 26 26.33 +58 31 59.6 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,2461238.7374,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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 07 17.2373 2461238.7374 12.51 11:28:47.36 +57:50:32.5
142.56841 56.02250 galactic UMa Second-epoch detections are separated by 0.6" and 7.1 pix
The object was found in VSX 1" Gaia DR3 857957620463391488
Type: ROT
# Max. Min./Amp. JD0 Period
13.220 G 13.250 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:47.36 +57:50:32.5: 13.43 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:47.36 +57:50:32.5: 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 07 17.2373* 11 28 47.36 +57 50 32.5 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 857957620463391488,2461238.7374,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 857957620463391488 20260717.2373 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 07 17.2373 2461238.7374 12.28 11:27:47.91 +57:49:50.5
142.77476 55.95767 galactic UMa Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:27:47.91 +57:49:50.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.597+/-0.035 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:27:47.91 +57:49:50.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:27:47.91 +57:49:50.5: 13.30 +/- 0.03 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 07 17.2373* 11 27 47.91 +57 49 50.5 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,2461238.7374,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.37 11:28:48.20 +58:07:41.8
142.27996 55.78669 galactic UMa Second-epoch detections are separated by 0.6" and 6.9 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 | 11:28:48.20 +58:07:41.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.368+/-0.035 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:48.20 +58:07:41.8: 13.44 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:48.20 +58:07:41.8: 13.40 +/- 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 07 17.2373* 11 28 48.20 +58 07 41.8 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,2461238.7374,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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 07 17.2373 2461238.7374 12.34 11:29:36.29 +57:43:42.9
142.52134 56.17764 galactic UMa Second-epoch detections are separated by 1.1" and 7.0 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 | 11:29:36.29 +57:43:42.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:36.29 +57:43:42.9: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:36.29 +57:43:42.9: 13.34 +/- 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 07 17.2373* 11 29 36.29 +57 43 42.9 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,2461238.7374,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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 07 17.2373 2461238.7374 12.95 12:38:42.08 +64:43:02.7
125.15791 52.35575 galactic Dra Second-epoch detections are separated by 3.2" 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 | 12:38:42.08 +64:43:02.7 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.037 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:42.08 +64:43:02.7: 14.22 +/- 0.07 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:42.08 +64:43:02.7: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 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,2461238.7374,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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 07 17.2373 2461238.7374 13.05 12:37:43.27 +64:51:08.5
125.30944 52.21252 galactic Dra Second-epoch detections are separated by 1.5" 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 | 12:37:43.27 +64:51:08.5 (user input) | T | P | (position from user input) J-Ks=0.518+/-0.030 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:37:43.27 +64:51:08.5: 14.12 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:37:43.27 +64:51:08.5: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461238.7374,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.64 11:28:17.23 +58:21:25.5
142.15327 55.55896 galactic UMa Second-epoch detections are separated by 1.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:28:17.23 +58:21:25.5 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.368+/-0.038 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:17.23 +58:21:25.5: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:17.23 +58:21:25.5: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 07 17.2373* 11 28 17.23 +58 21 25.5 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,2461238.7374,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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 07 17.2373 2461238.7374 12.78 12:34:46.39 +65:39:33.5
125.68170 51.37988 galactic Dra 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 | 12:34:46.39 +65:39:33.5 (user input) | T | P | (position from user input) J-Ks=0.464+/-0.028 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:34:46.39 +65:39:33.5: 13.66 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:34:46.39 +65:39:33.5: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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,2461238.7374,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.66 11:26:41.06 +58:29:43.3
142.32223 55.32668 galactic UMa Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:26:41.06 +58:29:43.3 (user input) | T | P | (position from user input) J-Ks=0.527+/-0.033 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:26:41.06 +58:29:43.3: 13.62 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:26:41.06 +58:29:43.3: 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 07 17.2373* 11 26 41.06 +58 29 43.3 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,2461238.7374,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.35 11:31:10.14 +57:30:57.4
142.42057 56.47080 galactic UMa Second-epoch detections are separated by 1.0" 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 | 11:31:10.14 +57:30:57.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:31:10.14 +57:30:57.4: 13.61 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:31:10.14 +57:30:57.4: 13.57 +/- 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 07 17.2373* 11 31 10.14 +57 30 57.4 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,2461238.7374,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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 07 17.2373 2461238.7374 12.96 12:31:57.76 +65:46:30.1
126.12023 51.23249 galactic Dra Second-epoch detections are separated by 0.7" 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 | 12:31:57.76 +65:46:30.1 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.033 (F)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:31:57.76 +65:46:30.1: 13.91 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:31:57.76 +65:46:30.1: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 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,2461238.7374,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.98 12:37:21.62 +66:03:24.4
125.20111 51.00940 galactic Dra 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 | 12:37:21.62 +66:03:24.4 (user input) | T | P | (position from user input) J-Ks=0.281+/-0.039 (F)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:37:21.62 +66:03:24.4: 14.04 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:37:21.62 +66:03:24.4: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.7374,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 13.01 12:36:49.11 +65:50:12.1
125.31981 51.22372 galactic Dra Second-epoch detections are separated by 2.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:49.11 +65:50:12.1 (user input) | T | P | (position from user input) J-Ks=0.593+/-0.029 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:36:49.11 +65:50:12.1: 14.06 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:36:49.11 +65:50:12.1: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.7374,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.79 12:38:44.10 +65:12:53.7
125.08701 51.86015 galactic Dra Second-epoch detections are separated by 0.4" and 6.2 pix
The object was found in VSX 1" GSC 04168-00008
Type: RRAB
# Max. Min./Amp. JD0 Period
13.600 V 14.600 V 2456091.66990 0.531010000000
The object was not found in astcheck.
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:44.10 +65:12:53.7: 14.04 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:44.10 +65:12:53.7: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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
GSC 04168-00008,2461238.7374,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 04168-00008 20260717.2373 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 07 17.2373 2461238.7374 12.19 11:28:18.22 +57:30:59.9
142.99493 56.25451 galactic UMa Second-epoch detections are separated by 0.9" and 6.9 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 | Large-amplitude variable Gaia DR2 857937932333356160 | 11:28:18.22 +57:30:59.9 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F2 (LAMOST DR5) J-Ks=0.352+/-0.034 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:18.22 +57:30:59.9: 13.11 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:18.22 +57:30:59.9: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2373* 11 28 18.22 +57 30 59.9 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
Large-amplitude variable Gaia DR2 857937932333356160,2461238.7374,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 857937932333356160 20260717.2373 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 07 17.2373 2461238.7374 12.53 11:31:20.76 +57:45:29.2
142.14394 56.28174 galactic UMa Second-epoch detections are separated by 1.4" and 7.0 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 | 11:31:20.76 +57:45:29.2 (user input) | T | P | (position from user input) J-Ks=0.734+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:31:20.76 +57:45:29.2: 13.61 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:31:20.76 +57:45:29.2: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 07 17.2373* 11 31 20.76 +57 45 29.2 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,2461238.7374,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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 07 17.2373 2461238.7374 12.56 11:30:03.81 +57:59:23.6
142.17005 55.99437 galactic UMa Second-epoch detections are separated by 2.6" 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 | 11:30:03.81 +57:59:23.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.383+/-0.034 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:30:03.81 +57:59:23.6: 13.59 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:30:03.81 +57:59:23.6: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2373* 11 30 03.81 +57 59 23.6 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,2461238.7374,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.91 12:35:44.12 +65:51:47.7
125.49188 51.18688 galactic Dra Second-epoch detections are separated by 1.1" 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 | 12:35:44.12 +65:51:47.7 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.031 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:35:44.12 +65:51:47.7: 13.92 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:35:44.12 +65:51:47.7: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461238.7374,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.88 12:38:50.23 +65:23:13.4
125.04774 51.68940 galactic Dra Second-epoch detections are separated by 0.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:38:50.23 +65:23:13.4 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.028 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:50.23 +65:23:13.4: 13.89 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:50.23 +65:23:13.4: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461238.7374,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.87 11:29:27.97 +57:54:25.7
142.37012 56.01918 galactic UMa Second-epoch detections are separated by 4.4" 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 | 11:29:27.97 +57:54:25.7 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.399+/-0.039 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:27.97 +57:54:25.7: 14.16 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:27.97 +57:54:25.7: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 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 07 17.2373* 11 29 27.97 +57 54 25.7 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,2461238.7374,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.08 11:29:00.56 +57:55:59.6
142.43403 55.96366 galactic UMa Second-epoch detections are separated by 0.6" and 6.9 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 | 11:29:00.56 +57:55:59.6 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:00.56 +57:55:59.6: 13.06 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:00.56 +57:55:59.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2373* 11 29 00.56 +57 55 59.6 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,2461238.7374,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 13.13 12:36:32.77 +66:05:21.0
125.32713 50.96977 galactic Dra Second-epoch detections are separated by 1.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:32.77 +66:05:21.0 (user input) | T | P | (position from user input) J-Ks=0.567+/-0.031 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:36:32.77 +66:05:21.0: 14.16 +/- 0.07 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:36:32.77 +66:05:21.0: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.7374,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.28 11:27:04.23 +58:20:37.4
142.39975 55.48034 galactic UMa Second-epoch detections are separated by 1.2" 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 | ATO J171.7726+58.3410 | 11:27:04.23 +58:20:37.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.443+/-0.032 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:27:04.23 +58:20:37.4: 13.27 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:27:04.23 +58:20:37.4: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 07 17.2373* 11 27 04.23 +58 20 37.4 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
ATO J171.7726+58.3410,2461238.7374,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J171.7726+58.3410 20260717.2373 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 13.04 12:34:59.17 +65:19:09.7
125.70285 51.72029 galactic Dra 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 | target | 12:34:59.17 +65:19:09.7 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.032 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:34:59.17 +65:19:09.7: 14.15 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:34:59.17 +65:19:09.7: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.7374,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.76 11:28:14.61 +58:13:06.1
142.29911 55.67073 galactic UMa Second-epoch detections are separated by 1.2" 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 | 11:28:14.61 +58:13:06.1 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.801+/-0.034 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:14.61 +58:13:06.1: 13.98 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:14.61 +58:13:06.1: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 07 17.2373* 11 28 14.61 +58 13 06.1 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,2461238.7374,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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 07 17.2373 2461238.7374 12.44 11:27:10.10 +58:09:44.7
142.56243 55.63710 galactic UMa Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:27:10.10 +58:09:44.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.333+/-0.033 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:27:10.10 +58:09:44.7: 13.56 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:27:10.10 +58:09:44.7: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 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 07 17.2373* 11 27 10.10 +58 09 44.7 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,2461238.7374,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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 07 17.2373 2461238.7374 12.81 12:36:53.03 +64:17:50.7
125.53853 52.75711 galactic Dra Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:53.03 +64:17:50.7 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.030 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:36:53.03 +64:17:50.7: 13.79 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:36:53.03 +64:17:50.7: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461238.7374,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.73 11:28:10.90 +58:03:52.7
142.46438 55.79336 galactic UMa Second-epoch detections are separated by 1.0" and 7.0 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 | 11:28:10.90 +58:03:52.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.364+/-0.038 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:10.90 +58:03:52.7: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:10.90 +58:03:52.7: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 07 17.2373* 11 28 10.90 +58 03 52.7 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,2461238.7374,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.82 12:38:49.99 +64:22:23.1
125.18045 52.70010 galactic Dra 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 | 12:38:49.99 +64:22:23.1 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:49.99 +64:22:23.1: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:49.99 +64:22:23.1: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461238.7374,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.28 11:26:28.15 +58:19:14.3
142.53753 55.45462 galactic UMa Second-epoch detections are separated by 0.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:26:28.15 +58:19:14.3 (user input) | T | P | (position from user input) J-Ks=0.292+/-0.029 (F)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:26:28.15 +58:19:14.3: 13.26 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:26:28.15 +58:19:14.3: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2373* 11 26 28.15 +58 19 14.3 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,2461238.7374,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 13.07 12:38:53.76 +64:50:03.8
125.10876 52.24082 galactic Dra 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 | 12:38:53.76 +64:50:03.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:53.76 +64:50:03.8: 14.31 +/- 0.07 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:53.76 +64:50:03.8: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.7374,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 11.66 11:29:32.03 +57:51:10.6
142.41086 56.06918 galactic UMa Second-epoch detections are separated by 0.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 857962740064405376 | 11:29:32.04 +57:51:09.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.610+/-0.032 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:32.03 +57:51:10.6: 12.66 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:32.03 +57:51:10.6: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2373* 11 29 32.03 +57 51 10.6 11.7 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 857962740064405376,2461238.7374,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 857962740064405376 20260717.2373 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.61 12:36:44.70 +66:04:26.4
125.29745 50.98671 galactic Dra Second-epoch detections are separated by 1.0" 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 | 12:36:44.70 +66:04:26.4 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.028 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:36:44.70 +66:04:26.4: 13.53 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:36:44.70 +66:04:26.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 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,2461238.7374,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.73 11:29:12.52 +57:53:52.7
142.43004 56.00769 galactic UMa Second-epoch detections are separated by 2.8" 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 | 11:29:12.52 +57:53:52.7 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.033 (K)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:12.52 +57:53:52.7: 13.97 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:12.52 +57:53:52.7: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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 07 17.2373* 11 29 12.52 +57 53 52.7 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,2461238.7374,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.59 11:32:08.38 +57:30:57.5
142.22333 56.54248 galactic UMa Second-epoch detections are separated by 1.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:32:08.38 +57:30:57.5 (user input) | T | P | (position from user input) J-Ks=0.279+/-0.033 (F)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:32:08.38 +57:30:57.5: 13.73 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:32:08.38 +57:30:57.5: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 07 17.2373* 11 32 08.38 +57 30 57.5 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,2461238.7374,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2373 2461238.7374 12.76 12:37:43.09 +65:16:38.0
125.25027 51.78923 galactic Dra 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 | 12:37:43.09 +65:16:38.0 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.030 (G)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:37:43.09 +65:16:38.0: 13.76 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:37:43.09 +65:16:38.0: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461238.7374,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2373 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
## 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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Last image: 2461238.73760000 17.07.2026 05:41:58.640 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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: 4 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 5987
Objects passed selection criteria: 5941
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 3403
Average stars matched: 3170 (93.1531 %)
Memory usage VmPeak: 115264 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 16 05:04:38 CDT 2026
VaST build number 1.0rc89-156-g3b0d8dc3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 17 01:39:03 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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Last image: 2461238.73760000 17.07.2026 05:41:58.640 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 88
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.21
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: 15 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 31510
Objects passed selection criteria: 31369
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 19068.2
Average stars matched: 17336.5 (90.9181 %)
Memory usage VmPeak: 136776 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 16 05:04:38 CDT 2026
VaST build number 1.0rc89-156-g3b0d8dc3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 17 01:40:55 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
SExtractor catalog cache: saved UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.cat to cache
SExtractor catalog cache: saved UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.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: 2461238.73710058
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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits exists and is non-empty
Saving wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits to local_wcs_cache/
'wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits' -> 'local_wcs_cache/wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits'
wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits exists and is non-empty
Saving wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits to local_wcs_cache/
'wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits' -> 'local_wcs_cache/wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits'
wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits exists and is non-empty
Saving wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits to local_wcs_cache/
'wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits' -> 'local_wcs_cache/wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits'
wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits exists and is non-empty
Saving wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits to local_wcs_cache/
'wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits' -> 'local_wcs_cache/wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits (1st reference image)
verification OK: wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Image size: 941.7'x627.1' 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: 12:00:03.732 +62:00:23.71 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-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits (1st new image)
verification OK: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
Image size: 937.7'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:07.901 +62:01:54.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:03.732 +62:00:23.71
Second-epoch image center 12:00:07.901 +62:01:54.96
Angular distance between the image centers 0.0266 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits (2nd new image)
verification OK: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
Image size: 937.7'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:04.172 +62:02:24.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:03.732 +62:00:23.71
Second-epoch image center 12:00:04.172 +62:02:24.00
Angular distance between the image centers 0.0334 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 12:00:07.901 +62:01:54.96
Second-epoch second image center 12:00:04.172 +62:02:24.00
Angular distance between the image centers 0.01087 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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits &> /tmp/tmp.2qvyKE9r2g
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits &> /tmp/tmp.wBEMhPo00Y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits &> /tmp/tmp.Pnu8Rp9DTB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits &> /tmp/tmp.eoIjOJC8Oa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
Found non-empty wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
The reference image (wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits) and catalog (wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat) found
'wcs_UMa-04-Q2b1x1_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 159.9761 to 198.4298 deg, Dec +55.2649 to +67.4535 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 159.9761 to 198.4298 deg, Dec 55.2649 to 67.4535 deg
Loaded 6571 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): 3978 out of 4192 total matches.
Matched with Tycho-2 4192 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 22.890450
a=0.000000 b=1.000000 c=22.890450
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
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 159.9761 to 198.4298 deg, Dec +55.2649 to +67.4535 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 159.9761 to 198.4298 deg, Dec 55.2649 to 67.4535 deg
Loaded 6571 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): 3978 out of 4192 total matches.
Matched with Tycho-2 4192 out of 7332 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits:
Forced-photometry filter: calibrated wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits -> calib.txt_param_ref_wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits (aperture=6.3)
Read 7282 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.9754 to 198.4299 deg, Dec +55.3321 to +67.4949 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 159.9754 to 198.4299 deg, Dec 55.3321 to 67.4949 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): 3981 out of 4179 total matches.
Matched with Tycho-2 4179 out of 7282 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits:
Forced-photometry filter: calibrated wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits -> calib.txt_param_ref_wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
2.2 pix UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
2.2 pix fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
2.2 pix fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
2.2 pix wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
2.2 pix wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Limiting magnitude estimates:
15.4 mag. UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
15.4 mag. UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
13.4 mag. fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
13.3 mag. fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2qvyKE9r2g (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits' -> 'wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS_IMAGE_NAME=wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS-calibrated image found: wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Checking if the catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat corresponding to the image wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits alredy exist and is non-empty...
Catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat corresponding to the image wcs_UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS catalog name: wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=506, bad_region=1672, passed=7332
Got 7332 stars (including 5274 good ones) from the SExtractor catalog wcs_UMa-04-Q2b1x1_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: 941.7'
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
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 977 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits N_match=979 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.404 sigma_q3_arcsec=0.349 sigma_q4_arcsec=0.333 n_q1=287 n_q2=162 n_q3=316 n_q4=214 worst_quadrant_to_overall_ratio=1.152
The image catalog is written to wcs_UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits -region wcs_UMa-04-Q2b1x1_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-Q2b1x1_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.wBEMhPo00Y (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits' -> 'wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS_IMAGE_NAME=wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS-calibrated image found: wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Checking if the catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat corresponding to the image wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits alredy exist and is non-empty...
Catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat corresponding to the image wcs_UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS catalog name: wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=494, bad_region=1659, passed=7282
Got 7282 stars (including 5242 good ones) from the SExtractor catalog wcs_UMa-04-Q2b1x1_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: 941.7'
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
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 5825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 5825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 5825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits N_match=978 sigma_overall_arcsec=0.419 sigma_q1_arcsec=0.479 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.382 sigma_q4_arcsec=0.346 n_q1=290 n_q2=162 n_q3=314 n_q4=212 worst_quadrant_to_overall_ratio=1.144
The image catalog is written to wcs_UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits -region wcs_UMa-04-Q2b1x1_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-Q2b1x1_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.Pnu8Rp9DTB (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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
WCS-calibrated image found: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
Checking if the catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
WCS catalog name: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=86, bad_region=175, passed=1383
Got 1383 stars (including 1132 good ones) from the SExtractor catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat
util/solve_plate_with_UCAC5 got 1383 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 1201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 1200 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 1200 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 969 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits N_match=969 sigma_overall_arcsec=0.386 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.587 sigma_q3_arcsec=0.456 sigma_q4_arcsec=0.429 n_q1=553 n_q2=25 n_q3=252 n_q4=139 worst_quadrant_to_overall_ratio=1.520
The image catalog is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits -region wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.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.eoIjOJC8Oa (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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
WCS_IMAGE_NAME=wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
WCS-calibrated image found: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
Checking if the catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
WCS catalog name: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=73, bad_region=83, passed=1265
Got 1265 stars (including 1112 good ones) from the SExtractor catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat
util/solve_plate_with_UCAC5 got 1265 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 1168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 1166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 1166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits N_match=971 sigma_overall_arcsec=0.404 sigma_q1_arcsec=0.373 sigma_q2_arcsec=0.543 sigma_q3_arcsec=0.466 sigma_q4_arcsec=0.419 n_q1=539 n_q2=23 n_q3=291 n_q4=118 worst_quadrant_to_overall_ratio=1.344
The image catalog is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits -region wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits sigma_overall=0.388 worst_q_ratio=1.152
ref2=UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits sigma_overall=0.419 worst_q_ratio=1.144
new1=fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits sigma_overall=0.386 worst_q_ratio=1.520
new2=fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits sigma_overall=0.404 worst_q_ratio=1.344
reference average sigma_overall=0.4035 worst_q_ratio=1.148
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278_astrometric_residuals.png (979 matched stars from wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279_astrometric_residuals.png (978 matched stars from wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149_astrometric_residuals.png (969 matched stars from wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150_astrometric_residuals.png (971 matched stars from wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits'
Saving fully-calibrated image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits'
Preparing the HTML report for the field UMa-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field UMa-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
SExtractor catalog cache: saved UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.cat to cache
SExtractor catalog cache: saved UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Creating symlink local_wcs_cache/wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits exists and is non-empty
wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits exists and is non-empty
wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits exists and is non-empty
wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits (1st reference image)
verification OK: wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Image size: 941.7'x627.1' 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: 12:00:03.732 +62:00:23.71 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-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits (1st new image)
verification OK: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
Image size: 937.7'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:07.901 +62:01:54.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:03.732 +62:00:23.71
Second-epoch image center 12:00:07.901 +62:01:54.96
Angular distance between the image centers 0.0266 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits (2nd new image)
verification OK: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
Image size: 937.7'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:04.172 +62:02:24.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:03.732 +62:00:23.71
Second-epoch image center 12:00:04.172 +62:02:24.00
Angular distance between the image centers 0.0334 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 12:00:07.901 +62:01:54.96
Second-epoch second image center 12:00:04.172 +62:02:24.00
Angular distance between the image centers 0.01087 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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits &> /tmp/tmp.HMvGydeEHe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits &> /tmp/tmp.vbBfUCzlUT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits &> /tmp/tmp.BBttPrWj9t
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits &> /tmp/tmp.uAeTKRbm8u
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
Found non-empty wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits and wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
The reference image (wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits) and catalog (wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat) found
'wcs_UMa-04-Q2b1x1_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 159.9761 to 198.6760 deg, Dec +55.2262 to +67.4863 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 159.9761 to 198.6760 deg, Dec 55.2262 to 67.4863 deg
Loaded 6640 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): 3750 out of 4197 total matches.
Matched with Tycho-2 4197 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 22.782250
a=0.000000 b=1.000000 c=22.782250
From vast_summary.log: estimated ref. image limiting mag.: -7.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
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 159.9761 to 198.6760 deg, Dec +55.2262 to +67.4863 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 159.9761 to 198.6760 deg, Dec 55.2262 to 67.4863 deg
Loaded 6640 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): 3750 out of 4197 total matches.
Matched with Tycho-2 4197 out of 37333 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits:
Forced-photometry filter: calibrated wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits -> calib.txt_param_ref_wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits (aperture=5.0)
Read 37494 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.9755 to 198.6753 deg, Dec +55.2659 to +67.4949 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 159.9755 to 198.6753 deg, Dec 55.2659 to 67.4949 deg
Loaded 6626 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): 3751 out of 4193 total matches.
Matched with Tycho-2 4193 out of 37494 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits:
Forced-photometry filter: calibrated wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits -> calib.txt_param_ref_wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 41 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
2.1 pix UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
2.2 pix fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
2.1 pix fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
2.1 pix wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
2.1 pix wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Limiting magnitude estimates:
15.6 mag. UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
15.6 mag. UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
13.4 mag. fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
13.3 mag. fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 13.0 (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.HMvGydeEHe (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits' -> 'wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS_IMAGE_NAME=wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS-calibrated image found: wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
Checking if the catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat corresponding to the image wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits alredy exist and is non-empty...
Catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat corresponding to the image wcs_UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits
WCS catalog name: wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1765, bad_region=7377, passed=37316
Got 37316 stars (including 28488 good ones) from the SExtractor catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits.wcscat
util/solve_plate_with_UCAC5 got 37316 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
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 30726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 30727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 30728 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits N_match=977 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.473 sigma_q2_arcsec=0.409 sigma_q3_arcsec=0.338 sigma_q4_arcsec=0.292 n_q1=275 n_q2=165 n_q3=324 n_q4=213 worst_quadrant_to_overall_ratio=1.239
The image catalog is written to wcs_UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits -region wcs_UMa-04-Q2b1x1_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-Q2b1x1_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.vbBfUCzlUT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits' -> 'wcs_UMa-04-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS_IMAGE_NAME=wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS-calibrated image found: wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
Checking if the catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat corresponding to the image wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits alredy exist and is non-empty...
Catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat corresponding to the image wcs_UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits
WCS catalog name: wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1739, bad_region=7420, passed=37478
Got 37478 stars (including 28617 good ones) from the SExtractor catalog wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits.wcscat
util/solve_plate_with_UCAC5 got 37478 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
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 30849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 30849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 30849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits N_match=977 sigma_overall_arcsec=0.410 sigma_q1_arcsec=0.485 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.344 n_q1=276 n_q2=167 n_q3=322 n_q4=212 worst_quadrant_to_overall_ratio=1.181
The image catalog is written to wcs_UMa-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits -region wcs_UMa-04-Q2b1x1_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-Q2b1x1_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.BBttPrWj9t (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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
WCS-calibrated image found: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
Checking if the catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
WCS catalog name: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=283, bad_region=861, passed=9194
Got 9194 stars (including 8109 good ones) from the SExtractor catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat
util/solve_plate_with_UCAC5 got 9194 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 8037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 963 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits N_match=963 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.347 sigma_q2_arcsec=0.610 sigma_q3_arcsec=0.416 sigma_q4_arcsec=0.395 n_q1=551 n_q2=23 n_q3=252 n_q4=137 worst_quadrant_to_overall_ratio=1.592
The image catalog is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits -region wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.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.uAeTKRbm8u (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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
WCS_IMAGE_NAME=wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
WCS-calibrated image found: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
Checking if the catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat corresponding to the image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
WCS catalog name: wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=222, bad_region=443, passed=8884
Got 8884 stars (including 8231 good ones) from the SExtractor catalog wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat
util/solve_plate_with_UCAC5 got 8884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits N_match=962 sigma_overall_arcsec=0.390 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.454 sigma_q3_arcsec=0.459 sigma_q4_arcsec=0.410 n_q1=540 n_q2=24 n_q3=285 n_q4=113 worst_quadrant_to_overall_ratio=1.177
The image catalog is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits -region wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.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-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-15_20.00sec_5.00C_LIGHT_0149.fits
Saving fully-calibrated image wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.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_2026-07-17_CI_UMa-04-Q2b1x1_004234_TTUQ2b1x1_2796465_2T8z5Ymg/wcs_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150.fits
Preparing the HTML report for the field UMa-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:17.23 +58:21:25.5: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:27:47.91 +57:49:50.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:48.20 +58:07:41.8: 13.44 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:42.08 +64:43:02.7: 14.22 +/- 0.07 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:47.36 +57:50:32.5: 13.43 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:26:26.33 +58:31:59.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:37:43.27 +64:51:08.5: 14.12 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:36.29 +57:43:42.9: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:37:37.50 +66:04:05.6: 13.98 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:27:47.91 +57:49:50.5: 13.30 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:17.23 +58:21:25.5: 13.66 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:48.20 +58:07:41.8: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:47.36 +57:50:32.5: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:42.08 +64:43:02.7: 14.07 +/- 0.06 detection
Forced photometry filter KEPT candidate at 11:27:47.91 +57:49:50.5: ref_mag=13.35 +/- 0.02 new_mean_mag=12.2780 delta=1.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 11:28:47.36 +57:50:32.5: ref_mag=13.44 +/- 0.02 new_mean_mag=12.5036 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 14.13 +/- 0.04
Forced photometry filter KEPT candidate at 12:38:42.08 +64:43:02.7: ref_mag=14.13 +/- 0.04 new_mean_mag=12.9259 delta=1.21 (need > 0.90)
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:26:26.33 +58:31:59.6: 13.54 +/- 0.03 detection
Forced photometry filter KEPT candidate at 11:28:17.23 +58:21:25.5: ref_mag=13.67 +/- 0.03 new_mean_mag=12.6476 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 11:28:48.20 +58:07:41.8: ref_mag=13.42 +/- 0.02 new_mean_mag=12.3681 delta=1.05 (need > 0.90)
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry filter KEPT candidate at 11:26:26.33 +58:31:59.6: ref_mag=13.51 +/- 0.02 new_mean_mag=12.5005 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:36.29 +57:43:42.9: 13.34 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:37:43.27 +64:51:08.5: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:34:46.39 +65:39:33.5: 13.66 +/- 0.04 detection
Forced photometry filter KEPT candidate at 11:29:36.29 +57:43:42.9: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3474 delta=1.02 (need > 0.90)
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Forced photometry filter KEPT candidate at 12:37:43.27 +64:51:08.5: ref_mag=14.07 +/- 0.04 new_mean_mag=13.0497 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:34:46.39 +65:39:33.5: 13.76 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:37:37.50 +66:04:05.6: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:46.39 +65:39:33.5: ref_mag=13.70 +/- 0.03 new_mean_mag=12.7727 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 12:37:37.50 +66:04:05.6: ref_mag=13.94 +/- 0.04 new_mean_mag=13.0207 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:26:41.06 +58:29:43.3: 13.62 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:26:41.06 +58:29:43.3: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry filter KEPT candidate at 11:26:41.06 +58:29:43.3: ref_mag=13.61 +/- 0.02 new_mean_mag=12.6634 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:31:10.14 +57:30:57.4: 13.61 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:31:57.76 +65:46:30.1: 13.91 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:37:21.62 +66:03:24.4: 14.04 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:31:10.14 +57:30:57.4: 13.57 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:31:57.76 +65:46:30.1: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 11:31:10.14 +57:30:57.4: ref_mag=13.59 +/- 0.03 new_mean_mag=12.3508 delta=1.24 (need > 0.90)
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:57.76 +65:46:30.1: ref_mag=13.87 +/- 0.03 new_mean_mag=12.9563 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:37:21.62 +66:03:24.4: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.04
Forced photometry filter KEPT candidate at 12:37:21.62 +66:03:24.4: ref_mag=14.05 +/- 0.04 new_mean_mag=12.9809 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:36:49.11 +65:50:12.1: 14.06 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:44.10 +65:12:53.7: 14.04 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:36:49.11 +65:50:12.1: 13.98 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:44.10 +65:12:53.7: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 12:36:49.11 +65:50:12.1: ref_mag=14.02 +/- 0.04 new_mean_mag=12.9755 delta=1.04 (need > 0.90)
Forced photometry filter KEPT candidate at 12:38:44.10 +65:12:53.7: ref_mag=13.94 +/- 0.04 new_mean_mag=12.7641 delta=1.17 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:18.22 +57:30:59.9: 13.11 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:18.22 +57:30:59.9: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 11:28:18.22 +57:30:59.9: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1709 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:31:20.76 +57:45:29.2: 13.61 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:31:20.76 +57:45:29.2: 13.51 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:30:03.81 +57:59:23.6: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Forced photometry filter KEPT candidate at 11:31:20.76 +57:45:29.2: ref_mag=13.56 +/- 0.02 new_mean_mag=12.5104 delta=1.05 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:30:03.81 +57:59:23.6: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 11:30:03.81 +57:59:23.6: ref_mag=13.62 +/- 0.03 new_mean_mag=12.5620 delta=1.06 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:35:44.12 +65:51:47.7: 13.92 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:35:44.12 +65:51:47.7: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Forced photometry filter KEPT candidate at 12:35:44.12 +65:51:47.7: ref_mag=13.89 +/- 0.03 new_mean_mag=12.9071 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:50.23 +65:23:13.4: 13.89 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:50.23 +65:23:13.4: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Forced photometry filter KEPT candidate at 12:38:50.23 +65:23:13.4: ref_mag=13.89 +/- 0.03 new_mean_mag=12.8953 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:27.97 +57:54:25.7: 14.16 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:27.97 +57:54:25.7: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry filter KEPT candidate at 11:29:27.97 +57:54:25.7: ref_mag=14.10 +/- 0.04 new_mean_mag=12.8796 delta=1.22 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:00.56 +57:55:59.6: 13.06 +/- 0.02 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:29:05.03 +65:29:45.9: 13.87 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:36:32.77 +66:05:21.0: 14.16 +/- 0.07 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:00.56 +57:55:59.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 11:29:00.56 +57:55:59.6: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0777 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:27:04.23 +58:20:37.4: 13.27 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:29:05.03 +65:29:45.9: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter REJECTED candidate at 12:29:05.03 +65:29:45.9: ref_mag=13.81 +/- 0.03 new_mean_mag=12.9094 delta=0.90 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:36:32.77 +66:05:21.0: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.05
Forced photometry filter KEPT candidate at 12:36:32.77 +66:05:21.0: ref_mag=14.14 +/- 0.05 new_mean_mag=13.1311 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:27:04.23 +58:20:37.4: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 11:27:04.23 +58:20:37.4: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2856 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:34:59.17 +65:19:09.7: 14.15 +/- 0.06 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:27:10.10 +58:09:44.7: 13.56 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:34:59.17 +65:19:09.7: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Forced photometry filter KEPT candidate at 12:34:59.17 +65:19:09.7: ref_mag=14.02 +/- 0.04 new_mean_mag=13.0018 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:14.61 +58:13:06.1: 13.98 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:36:53.03 +64:17:50.7: 13.79 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:27:10.10 +58:09:44.7: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 11:27:10.10 +58:09:44.7: ref_mag=13.57 +/- 0.03 new_mean_mag=12.4318 delta=1.14 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:14.61 +58:13:06.1: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
Forced photometry filter KEPT candidate at 11:28:14.61 +58:13:06.1: ref_mag=14.00 +/- 0.04 new_mean_mag=12.7888 delta=1.21 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:36:53.03 +64:17:50.7: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 12:36:53.03 +64:17:50.7: ref_mag=13.79 +/- 0.03 new_mean_mag=12.8115 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:28:10.90 +58:03:52.7: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:28:10.90 +58:03:52.7: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter KEPT candidate at 11:28:10.90 +58:03:52.7: ref_mag=13.85 +/- 0.03 new_mean_mag=12.7384 delta=1.11 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:49.99 +64:22:23.1: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:49.99 +64:22:23.1: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 12:38:49.99 +64:22:23.1: ref_mag=13.79 +/- 0.03 new_mean_mag=12.8000 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:26:28.15 +58:19:14.3: 13.26 +/- 0.03 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:26:28.15 +58:19:14.3: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 11:26:28.15 +58:19:14.3: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2861 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:38:53.76 +64:50:03.8: 14.31 +/- 0.07 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:38:53.76 +64:50:03.8: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.05
Forced photometry filter KEPT candidate at 12:38:53.76 +64:50:03.8: ref_mag=14.30 +/- 0.05 new_mean_mag=13.0702 delta=1.23 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:32.03 +57:51:10.6: 12.66 +/- 0.01 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:36:44.70 +66:04:26.4: 13.53 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:32.03 +57:51:10.6: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 11:29:32.03 +57:51:10.6: ref_mag=12.66 +/- 0.01 new_mean_mag=11.6590 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:36:44.70 +66:04:26.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 12:36:44.70 +66:04:26.4: ref_mag=13.57 +/- 0.03 new_mean_mag=12.6041 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:29:12.52 +57:53:52.7: 13.97 +/- 0.05 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 11:32:08.38 +57:30:57.5: 13.73 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:29:12.52 +57:53:52.7: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 11:29:12.52 +57:53:52.7: ref_mag=13.94 +/- 0.04 new_mean_mag=12.7448 delta=1.19 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 11:32:08.38 +57:30:57.5: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 11:32:08.38 +57:30:57.5: ref_mag=13.70 +/- 0.03 new_mean_mag=12.6033 delta=1.10 (need > 0.90)
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-33-00_20.00sec_-14.90C_LIGHT_0278.fits at 12:37:43.09 +65:16:38.0: 13.76 +/- 0.04 detection
Forced photometry on wcs_UMa-04-Q2b1x1_2026-02-22_00-34-07_20.00sec_-14.90C_LIGHT_0279.fits at 12:37:43.09 +65:16:38.0: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 12:37:43.09 +65:16:38.0: ref_mag=13.75 +/- 0.03 new_mean_mag=12.7573 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out04544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35372.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 70s
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: 23s
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Considering the candidate 29532_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 29532_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 08329_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 08329_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 05858_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 05858_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 05865_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
The candidate 05865_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150 did not pass the final checks
**** FOUND 11:28:48.82 +57:50:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05937_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 05937_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 06809_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 06809_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 05410_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 05410_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 34019_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 34019_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 33542_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 33542_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 07576_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 07576_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 31060_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 31060_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 08203_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 08203_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 04639_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 04639_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 30616_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 30616_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 29707_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 29707_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 25640_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 25640_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 32394_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 32394_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 04912_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 04912_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 05333_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 05333_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 06218_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 06218_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 25610_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 25610_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 31848_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 31848_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 06012_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 06012_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 30644_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
The candidate 30644_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (36.8") between the two second-epoch detections
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Considering the candidate 06134_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 06134_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 31619_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
The candidate 31619_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150 did not pass the final checks
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Considering the candidate 29315_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 29315_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 07635_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 07635_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 31900_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 31900_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 07142_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 07142_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 07070_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 07070_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 35372_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 35372_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 06667_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 06667_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 26220_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 26220_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 07631_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 07631_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 26000_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 26000_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 05792_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 05792_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 29156_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 29156_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 06013_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 06013_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 04544_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 04544_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
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Considering the candidate 32301_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
Preparing report for the candidate 32301_fd_UMa-04-Q2b1x1_2026-07-17_00-41-58_20.00sec_4.90C_LIGHT_0150
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 97s
Prepared the HTML report for the field UMa-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:32:08.38 +57:30:57.5
11:31:10.14 +57:30:57.4
11:28:18.22 +57:30:59.9
11:31:20.76 +57:45:29.2
11:29:36.29 +57:43:42.9
11:29:32.03 +57:51:10.6
11:28:47.36 +57:50:32.5
11:27:47.91 +57:49:50.5
11:29:27.97 +57:54:25.7
11:29:12.52 +57:53:52.7
11:29:00.56 +57:55:59.6
11:30:03.81 +57:59:23.6
11:28:10.90 +58:03:52.7
11:28:48.20 +58:07:41.8
11:27:10.10 +58:09:44.7
11:28:14.61 +58:13:06.1
11:28:17.23 +58:21:25.5
11:26:28.15 +58:19:14.3
11:27:04.23 +58:20:37.4
11:26:41.06 +58:29:43.3
11:26:26.33 +58:31:59.6
12:35:44.12 +65:51:47.7
12:36:49.11 +65:50:12.1
12:38:53.76 +64:50:03.8
12:38:49.99 +64:22:23.1
12:36:44.70 +66:04:26.4
12:36:32.77 +66:05:21.0
12:37:37.50 +66:04:05.6
12:37:21.62 +66:03:24.4
12:31:57.76 +65:46:30.1
12:34:46.39 +65:39:33.5
12:38:50.23 +65:23:13.4
12:34:59.17 +65:19:09.7
12:37:43.09 +65:16:38.0
12:38:44.10 +65:12:53.7
12:37:43.27 +64:51:08.5
12:38:42.08 +64:43:02.7
12:36:53.03 +64:17:50.7
########### Completed UMa-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
12:37:37.50 +66:04:05.6
11:26:26.33 +58:31:59.6
11:28:47.36 +57:50:32.5
11:27:47.91 +57:49:50.5
11:28:48.20 +58:07:41.8
11:29:36.29 +57:43:42.9
12:38:42.08 +64:43:02.7
12:37:43.27 +64:51:08.5
11:28:17.23 +58:21:25.5
12:34:46.39 +65:39:33.5
11:26:41.06 +58:29:43.3
11:31:10.14 +57:30:57.4
12:31:57.76 +65:46:30.1
12:37:21.62 +66:03:24.4
12:36:49.11 +65:50:12.1
12:38:44.10 +65:12:53.7
11:28:18.22 +57:30:59.9
11:31:20.76 +57:45:29.2
11:30:03.81 +57:59:23.6
12:35:44.12 +65:51:47.7
12:38:50.23 +65:23:13.4
11:29:27.97 +57:54:25.7
11:29:00.56 +57:55:59.6
12:36:32.77 +66:05:21.0
11:27:04.23 +58:20:37.4
12:34:59.17 +65:19:09.7
11:28:14.61 +58:13:06.1
11:27:10.10 +58:09:44.7
12:36:53.03 +64:17:50.7
11:28:10.90 +58:03:52.7
12:38:49.99 +64:22:23.1
11:26:28.15 +58:19:14.3
12:38:53.76 +64:50:03.8
11:29:32.03 +57:51:10.6
12:36:44.70 +66:04:26.4
11:29:12.52 +57:53:52.7
11:32:08.38 +57:30:57.5
12:37:43.09 +65:16:38.0
###################################################################################
12:37:37.50 +66:04:05.6 -- not an asteroid (will add it to exclusion list)
11:26:26.33 +58:31:59.6 -- not an asteroid (will add it to exclusion list)
11:28:47.36 +57:50:32.5 -- not an asteroid (will add it to exclusion list)
11:27:47.91 +57:49:50.5 -- not an asteroid (will add it to exclusion list)
11:28:48.20 +58:07:41.8 -- not an asteroid (will add it to exclusion list)
11:29:36.29 +57:43:42.9 -- not an asteroid (will add it to exclusion list)
12:38:42.08 +64:43:02.7 -- not an asteroid (will add it to exclusion list)
12:37:43.27 +64:51:08.5 -- not an asteroid (will add it to exclusion list)
11:28:17.23 +58:21:25.5 -- not an asteroid (will add it to exclusion list)
12:34:46.39 +65:39:33.5 -- not an asteroid (will add it to exclusion list)
11:26:41.06 +58:29:43.3 -- not an asteroid (will add it to exclusion list)
11:31:10.14 +57:30:57.4 -- not an asteroid (will add it to exclusion list)
12:31:57.76 +65:46:30.1 -- not an asteroid (will add it to exclusion list)
12:37:21.62 +66:03:24.4 -- not an asteroid (will add it to exclusion list)
12:36:49.11 +65:50:12.1 -- not an asteroid (will add it to exclusion list)
12:38:44.10 +65:12:53.7 -- not an asteroid (will add it to exclusion list)
11:28:18.22 +57:30:59.9 -- not an asteroid (will add it to exclusion list)
11:31:20.76 +57:45:29.2 -- not an asteroid (will add it to exclusion list)
11:30:03.81 +57:59:23.6 -- not an asteroid (will add it to exclusion list)
12:35:44.12 +65:51:47.7 -- not an asteroid (will add it to exclusion list)
12:38:50.23 +65:23:13.4 -- not an asteroid (will add it to exclusion list)
11:29:27.97 +57:54:25.7 -- not an asteroid (will add it to exclusion list)
11:29:00.56 +57:55:59.6 -- not an asteroid (will add it to exclusion list)
12:36:32.77 +66:05:21.0 -- not an asteroid (will add it to exclusion list)
11:27:04.23 +58:20:37.4 -- not an asteroid (will add it to exclusion list)
12:34:59.17 +65:19:09.7 -- not an asteroid (will add it to exclusion list)
11:28:14.61 +58:13:06.1 -- not an asteroid (will add it to exclusion list)
11:27:10.10 +58:09:44.7 -- not an asteroid (will add it to exclusion list)
12:36:53.03 +64:17:50.7 -- not an asteroid (will add it to exclusion list)
11:28:10.90 +58:03:52.7 -- not an asteroid (will add it to exclusion list)
12:38:49.99 +64:22:23.1 -- not an asteroid (will add it to exclusion list)
11:26:28.15 +58:19:14.3 -- not an asteroid (will add it to exclusion list)
12:38:53.76 +64:50:03.8 -- not an asteroid (will add it to exclusion list)
11:29:32.03 +57:51:10.6 -- not an asteroid (will add it to exclusion list)
12:36:44.70 +66:04:26.4 -- not an asteroid (will add it to exclusion list)
11:29:12.52 +57:53:52.7 -- not an asteroid (will add it to exclusion list)
11:32:08.38 +57:30:57.5 -- not an asteroid (will add it to exclusion list)
12:37:43.09 +65:16:38.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
11:26:26.33 +58:31:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:26:28.15 +58:19:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:26:41.06 +58:29:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:27:04.23 +58:20:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:27:10.10 +58:09:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:27:47.91 +57:49:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:10.90 +58:03:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:14.61 +58:13:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:17.23 +58:21:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:18.22 +57:30:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:47.36 +57:50:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:48.20 +58:07:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:29:00.56 +57:55:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:29:12.52 +57:53:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:29:27.97 +57:54:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:29:32.03 +57:51:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:29:36.29 +57:43:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:30:03.81 +57:59:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:31:10.14 +57:30:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:31:20.76 +57:45:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:32:08.38 +57:30:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:31:57.76 +65:46:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:46.39 +65:39:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:59.17 +65:19:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:44.12 +65:51:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:32.77 +66:05:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:44.70 +66:04:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:49.11 +65:50:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:53.03 +64:17:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:21.62 +66:03:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:37.50 +66:04:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:43.09 +65:16:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:43.27 +64:51:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:42.08 +64:43:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:44.10 +65:12:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:49.99 +64:22:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:50.23 +65:23:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:53.76 +64:50:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
11:26:26.33 +58:31:59.6 -- not a known variable star
11:26:28.15 +58:19:14.3 -- not a known variable star
11:26:41.06 +58:29:43.3 -- not a known variable star
11:27:04.23 +58:20:37.4 -- not a known variable star
11:27:10.10 +58:09:44.7 -- not a known variable star
11:27:47.91 +57:49:50.5 -- not a known variable star
11:28:10.90 +58:03:52.7 -- not a known variable star
11:28:14.61 +58:13:06.1 -- not a known variable star
11:28:17.23 +58:21:25.5 -- not a known variable star
11:28:18.22 +57:30:59.9 -- not a known variable star
11:28:47.36 +57:50:32.5 -- a known variable star
11:28:48.20 +58:07:41.8 -- not a known variable star
11:29:00.56 +57:55:59.6 -- not a known variable star
11:29:12.52 +57:53:52.7 -- not a known variable star
11:29:27.97 +57:54:25.7 -- not a known variable star
11:29:32.03 +57:51:10.6 -- not a known variable star
11:29:36.29 +57:43:42.9 -- not a known variable star
11:30:03.81 +57:59:23.6 -- not a known variable star
11:31:10.14 +57:30:57.4 -- not a known variable star
11:31:20.76 +57:45:29.2 -- not a known variable star
11:32:08.38 +57:30:57.5 -- not a known variable star
12:31:57.76 +65:46:30.1 -- not a known variable star
12:34:46.39 +65:39:33.5 -- not a known variable star
12:34:59.17 +65:19:09.7 -- not a known variable star
12:35:44.12 +65:51:47.7 -- not a known variable star
12:36:32.77 +66:05:21.0 -- not a known variable star
12:36:44.70 +66:04:26.4 -- not a known variable star
12:36:49.11 +65:50:12.1 -- not a known variable star
12:36:53.03 +64:17:50.7 -- not a known variable star
12:37:21.62 +66:03:24.4 -- not a known variable star
12:37:37.50 +66:04:05.6 -- not a known variable star
12:37:43.09 +65:16:38.0 -- not a known variable star
12:37:43.27 +64:51:08.5 -- not a known variable star
12:38:42.08 +64:43:02.7 -- not a known variable star
12:38:44.10 +65:12:53.7 -- a known variable star
12:38:49.99 +64:22:23.1 -- not a known variable star
12:38:50.23 +65:23:13.4 -- not a known variable star
12:38:53.76 +64:50:03.8 -- not a known variable star
Found 36 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
38 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
11:26:26.33 +58:31:59.6
11:26:28.15 +58:19:14.3
11:26:41.06 +58:29:43.3
11:27:04.23 +58:20:37.4
11:27:10.10 +58:09:44.7
11:27:47.91 +57:49:50.5
11:28:10.90 +58:03:52.7
11:28:14.61 +58:13:06.1
11:28:17.23 +58:21:25.5
11:28:18.22 +57:30:59.9
11:28:47.36 +57:50:32.5
11:28:48.20 +58:07:41.8
11:29:00.56 +57:55:59.6
11:29:12.52 +57:53:52.7
11:29:27.97 +57:54:25.7
11:29:32.03 +57:51:10.6
11:29:36.29 +57:43:42.9
11:30:03.81 +57:59:23.6
11:31:10.14 +57:30:57.4
11:31:20.76 +57:45:29.2
11:32:08.38 +57:30:57.5
12:31:57.76 +65:46:30.1
12:34:46.39 +65:39:33.5
12:34:59.17 +65:19:09.7
12:35:44.12 +65:51:47.7
12:36:32.77 +66:05:21.0
12:36:44.70 +66:04:26.4
12:36:49.11 +65:50:12.1
12:36:53.03 +64:17:50.7
12:37:21.62 +66:03:24.4
12:37:37.50 +66:04:05.6
12:37:43.09 +65:16:38.0
12:37:43.27 +64:51:08.5
12:38:42.08 +64:43:02.7
12:38:44.10 +65:12:53.7
12:38:49.99 +64:22:23.1
12:38:50.23 +65:23:13.4
12:38:53.76 +64:50:03.8
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461238.73710058 -observatory V36
07:14:37.18 +17:23:34.4 Mercury (4.4mag)
10:39:56.39 +09:34:25.7 Venus (-4.2mag)
04:44:35.12 +22:12:08.1 Mars (1.3mag)
08:22:56.78 +19:51:18.3 Jupiter (-1.8mag)
00:56:27.62 +03:22:13.7 Saturn (0.7mag)
04:08:30.08 +20:48:27.6 Uranus (5.8mag)
00:16:56.82 +00:19:47.4 Neptune (7.7mag)
20:30:16.26 -23:21:02.2 Pluto (14.4mag)
10:16:06.04 +09:35:23.6 Moon (-9.0mag)
-rw-r--r-- 1 apache apache 361 Jul 17 01:39 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461238.73710058:
08:22:59.98 +19:51:08.0 Io (6.0mag)
08:22:55.58 +19:51:24.6 Europa (6.3mag)
08:23:12.20 +19:50:21.2 Ganymede (5.6mag)
08:22:30.52 +19:52:57.6 Callisto (6.8mag)
08:21:10.10 +19:38:31.7 Himalia (15.7mag)
08:23:00.09 +19:51:05.9 Thebe (16.6mag)
08:20:30.96 +19:41:28.8 Elara (17.7mag)
08:26:40.97 +19:41:48.5 Pasiphae (17.9mag)
08:27:30.65 +19:57:25.4 Carme (19.0mag)
00:56:39.59 +03:22:09.3 Titan (8.5mag)
00:56:32.61 +03:22:09.2 Rhea (9.8mag)
00:55:52.87 +03:20:12.3 Iapetus (11.2mag)
00:56:13.70 +03:22:15.9 Hyperion (14.5mag)
00:56:19.14 +03:18:27.4 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 17 01:39 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461238.73710058:
17:57:04.21 -31:22:21.2 JWST
19:49:12.76 -03:55:26.0 Chandra
09:11:55.51 -52:03:55.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 17 01:39 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461238.73710058 -observatory V36
02:45:54.82 +15:13:31.8 17.8mag P/1996 R2 (Lagerkvist)
18:12:51.93 -34:31:30.6 13.8mag P/2010 H2 (Vales)
06:32:32.78 -68:15:48.2 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:09.78 +32:33:59.2 17.6mag C/2017 K2 (PANSTARRS)
02:23:26.65 +19:51:39.3 15.7mag P/2021 N1 (ZTF)
22:55:12.29 +32:14:21.8 17.3mag C/2022 E2 (ATLAS)
06:20:11.08 +26:51:30.9 16.7mag C/2022 N2 (PANSTARRS)
10:01:33.90 +29:28:15.4 16.9mag C/2022 QE78 (ATLAS)
09:14:12.67 +05:07:05.3 17.9mag C/2022 R6 (PANSTARRS)
18:03:07.85 +21:00:07.2 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:04.97 -11:33:25.8 17.8mag P/2023 B1 (PANSTARRS)
21:40:37.66 +67:30:50.9 17.8mag C/2023 H5 (Lemmon)
16:17:59.02 -10:47:29.2 14.0mag C/2023 R1 (PANSTARRS)
08:12:45.85 +66:05:22.6 17.9mag C/2024 A1 (ATLAS)
07:41:43.46 +30:20:42.7 14.8mag C/2024 E1 (Wierzchos)
15:13:13.37 +15:28:58.8 17.6mag C/2024 G6 (ATLAS)
19:32:22.12 +40:38:49.4 13.7mag C/2024 J3 (ATLAS)
21:40:05.38 +46:59:39.1 17.8mag C/2024 R4 (PANSTARRS)
04:56:04.46 -13:30:26.3 15.7mag C/2024 T5 (ATLAS)
06:40:11.39 +27:55:10.1 18.0mag C/2025 J1 (Borisov)
07:18:59.85 -13:31:53.7 16.8mag C/2025 R3 (PANSTARRS)
10:04:14.42 +22:07:38.9 17.6mag C/2025 V2 (Rankin)
12:47:06.68 +03:37:31.8 17.1mag C/2025 Y1 (ATLAS)
16:33:32.80 +79:08:51.0 17.2mag C/2026 A2 (Bok)
02:53:10.31 +45:31:31.6 16.8mag C/2026 B2 (Sun-Gao)
11:30:03.18 +05:42:16.8 17.0mag A/2026 E1
21:29:37.53 -17:41:33.7 7.1mag 10P/Tempel
11:16:47.20 -02:11:43.6 16.2mag 29P/Schwassmann-Wachmann
04:10:00.37 +30:17:24.3 17.9mag 47P/Ashbrook-Jackson
10:22:25.98 +11:48:22.6 17.1mag 63P/Wild
00:51:03.36 -05:02:46.7 15.5mag 65P/Gunn
04:44:00.63 +20:29:24.0 13.7mag 78P/Gehrels
02:33:08.05 +11:31:06.0 16.3mag 88P/Howell
06:55:48.61 +30:04:00.2 15.8mag 93P/Lovas
04:43:29.79 +31:19:14.1 16.7mag 114P/Wiseman-Skiff
08:25:30.76 +29:53:47.6 15.2mag 123P/West-Hartley
11:01:03.02 -01:36:13.3 16.9mag 124P/Mrkos
05:02:44.59 +20:59:19.6 16.2mag 128P/Shoemaker-Holt
05:49:10.02 +19:37:54.8 17.8mag 131P/Mueller
07:38:12.09 +15:29:39.3 16.4mag 141P-D/Machholz
03:19:28.00 -20:33:41.3 15.1mag 161P/Hartley-IRAS
05:57:54.53 +35:19:00.2 15.4mag 162P/SidingSpring
18:43:21.23 +19:43:15.4 14.1mag 169P/NEAT
01:57:12.98 +08:18:50.1 17.6mag 220P/McNaught
16:35:30.67 -08:41:27.6 17.2mag 235P/LINEAR
08:59:42.27 +32:38:39.7 18.0mag 240P/NEAT
20:38:36.68 -50:57:47.1 17.8mag 259P/Garradd
02:18:41.32 +15:18:41.9 15.6mag 260P/McNaught
05:58:11.81 +37:19:41.9 17.4mag 295P/LINEAR
15:06:30.95 +05:25:26.9 17.6mag 391P/Kowalski
08:40:48.86 +19:23:26.6 17.9mag 450P/LONEOS
08:02:31.72 +38:38:23.0 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 17 01:39 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:33:53.06 -07:15:00.80 ASASSN-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
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 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
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
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
19:33:53.06 -07:15:00.80 2026-07-14.15 15.5
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
-rw-r--r-- 1 apache apache 5.6K Jul 17 01:39 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
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
-rw-r--r-- 1 apache apache 189K Jul 17 01:39 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:27:50.004 -06:44:08.56 AT 2026svd 2026-06-26.40 23.3852
04:22:38.209 -47:20:55.00 AT 2026svc 2026-06-26.43 22.5609
21:50:00.261 -07:57:05.98 AT 2026svb 2026-06-26.41 23.0326
00:44:37.185 -43:22:31.83 AT 2026sva 2026-06-26.42 21.6706
21:35:19.036 -19:34:24.34 AT 2026suz 2026-06-26.41 23.3439
22:40:47.013 -09:25:04.67 AT 2026suy 2026-06-26.40 23.289
22:05:53.553 -08:24:29.60 AT 2026sux 2026-06-26.41 22.2593
22:33:25.333 -02:10:00.75 AT 2026suw 2026-06-26.40 22.6919
22:01:05.082 -07:26:52.26 AT 2026suv 2026-06-26.41 22.9876
22:30:12.816 -04:52:34.67 AT 2026suu 2026-06-26.40 21.9579
21:54:55.644 -07:45:32.24 AT 2026sut 2026-06-26.41 21.0171
18:17:40.907 -50:01:40.94 AT 2026sus 2026-07-07.95 19.363
20:17:07.701 -31:44:39.62 SN 2026sur 2026-07-08.18 19.091
03:21:24.733 -45:31:36.65 AT 2026suq 2026-07-08.14 18.759
21:15:50.298 -66:09:30.96 AT 2026sup 2026-07-07.05 18.911
22:32:27.822 -20:22:41.23 AT 2026suo 2026-07-06.46 19.8035
04:03:27.102 -57:43:47.16 AT 2026sun 2026-07-08.15 18.325
23:58:57.947 -03:02:20.39 AT 2026sum 2026-07-08.38 19.6555
00:36:59.677 +43:01:07.64 AT 2026sul 2026-07-05.38 20.0025
14:33:14.800 +42:54:37.00 AT 2026suk 2026-06-30.71 21.4
-rw-r--r-- 1 apache apache 89K Jul 17 01:39 tns_transients_list.txt
