This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.17 06:09:55.06 +16:35:39.8
193.48076 -1.34372 galactic Ori Second-epoch detections are separated by 1.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.4739+16.5916 | 06:09:55.05 +16:35:39.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.176+/-0.034 (F)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:09:55.06 +16:35:39.8: 12.11 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:09:55.06 +16:35:39.8: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 09 55.06 +16 35 39.8 11.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.4739+16.5916,2461293.9879,11.17,0.05,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 J092.4739+16.5916 20260910.4879 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.77 06:07:01.43 +16:16:38.4
193.42189 -2.10434 galactic Ori Second-epoch detections are separated by 1.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:07:01.43 +16:16:38.4 (user input) | T | P | (position from user input) SpType: A9V (LAMOST DR5) J-Ks=0.248+/-0.031 (F)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:07:01.43 +16:16:38.4: 12.96 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:07:01.43 +16:16:38.4: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 07 01.43 +16 16 38.4 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9879,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4879 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.74 06:18:24.19 +11:14:16.6
199.17247 -2.09321 galactic Ori Second-epoch detections are separated by 1.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:18:24.19 +11:14:16.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.353+/-0.034 (G)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:24.19 +11:14:16.6: 12.81 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:24.19 +11:14:16.6: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 18 24.19 +11 14 16.6 11.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9879,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4879 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.65 06:08:09.05 +16:24:31.6
193.43824 -1.80416 galactic Ori Second-epoch detections are separated by 1.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:08:09.05 +16:24:31.6 (user input) | T | P | (position from user input) J-Ks=0.191+/-0.026 (F)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:08:09.05 +16:24:31.6: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:08:09.05 +16:24:31.6: 12.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 08 09.05 +16 24 31.6 11.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9879,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4879 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.79 06:20:28.28 +17:55:33.4
193.51229 1.50584 galactic Gem Second-epoch detections are separated by 0.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.1070+17.9284 | 06:20:28.28 +17:55:33.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.160+/-0.034 (F)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:28.28 +17:55:33.4: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:28.28 +17:55:33.4: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.1070+17.9284,2461293.9879,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.1070+17.9284 20260910.4879 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.62 06:05:44.58 +15:59:44.1
193.51838 -2.51018 galactic Ori Second-epoch detections are separated by 1.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.4395+15.9949 | 06:05:44.58 +15:59:44.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.345+/-0.030 (G)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:05:44.58 +15:59:44.1: 12.76 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:05:44.58 +15:59:44.1: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 05 44.58 +15 59 44.1 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.4395+15.9949,2461293.9879,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.4395+15.9949 20260910.4879 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.60 06:06:51.25 +16:02:04.1
193.61446 -2.25800 galactic Ori Second-epoch detections are separated by 1.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:06:51.25 +16:02:04.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.313+/-0.032 (F)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:51.25 +16:02:04.1: 12.69 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:51.25 +16:02:04.1: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 06 51.25 +16 02 04.1 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9879,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4879 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.62 06:18:31.55 +11:13:54.5
199.19211 -2.06959 galactic Ori Second-epoch detections are separated by 1.6" and 8.6 pix
The object was found in VSX22" ZTF J061832.34+111412.7
Type: EW
# Max. Min./Amp. JD0 Period
13.478 r Y 0.425 r 2458427.93790 0.347569000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:31.55 +11:13:54.5: 12.65 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:31.55 +11:13:54.5: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 18 31.55 +11 13 54.5 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J061832.34+111412.7,2461293.9879,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J061832.34+111412.7 20260910.4879 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.63 06:08:46.97 +16:33:36.5
193.37922 -1.59829 galactic Ori Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.470 Kilia 157 39 162 15.3 0 0
ATTENTION: measured mag 11.63 is 3.7 mag brighter than the predicted asteroid brightness 15.3 - the transient may be an unrelated new object!
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:08:46.97 +16:33:36.5: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:08:46.97 +16:33:36.5: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 08 46.97 +16 33 36.5 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461293.9879,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260910.4879 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.62 06:07:08.35 +16:15:19.9
193.45443 -2.09075 galactic Ori Second-epoch detections are separated by 1.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3349031913340336384 | 06:07:08.30 +16:15:19.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.843+/-0.028 (M)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:07:08.35 +16:15:19.9: 12.62 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:07:08.35 +16:15:19.9: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 07 08.35 +16 15 19.9 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349031913340336384,2461293.9879,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3349031913340336384 20260910.4879 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.40 06:06:22.32 +16:01:33.9
193.56540 -2.36331 galactic Ori Second-epoch detections are separated by 1.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3349001711130314752 | 06:06:22.29 +16:01:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.356+/-0.030 (G)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:22.32 +16:01:33.9: 12.60 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:22.32 +16:01:33.9: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 06 22.32 +16 01 33.9 11.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349001711130314752,2461293.9879,11.40,0.05,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 3349001711130314752 20260910.4879 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.68 06:09:43.53 +16:47:47.2
193.28156 -1.28640 galactic Ori Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3349170353022116992 | 06:09:43.59 +16:47:47.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.266+/-0.034 (F)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:09:43.53 +16:47:47.2: 12.56 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:09:43.53 +16:47:47.2: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 09 43.53 +16 47 47.2 11.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349170353022116992,2461293.9879,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3349170353022116992 20260910.4879 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.47 06:06:44.69 +15:57:55.3
193.66212 -2.31456 galactic Ori Second-epoch detections are separated by 1.8" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3349000306677760384 | 06:06:44.71 +15:57:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.277+/-0.034 (F)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:44.69 +15:57:55.3: 12.55 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:44.69 +15:57:55.3: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 06 44.69 +15 57 55.3 11.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349000306677760384,2461293.9879,11.47,0.05,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 3349000306677760384 20260910.4879 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.48 06:06:12.32 +16:00:13.0
193.56554 -2.40923 galactic Ori Second-epoch detections are separated by 0.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3349003051160111360 | 06:06:12.32 +16:00:12.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.338+/-0.030 (G)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:12.32 +16:00:13.0: 12.45 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:12.32 +16:00:13.0: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 06 12.32 +16 00 13.0 11.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349003051160111360,2461293.9879,11.48,0.05,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 3349003051160111360 20260910.4879 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.40 06:09:20.62 +16:16:36.6
193.69235 -1.61766 galactic Ori Second-epoch detections are separated by 1.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3346122743010575616 | 06:09:20.62 +16:16:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.373+/-0.034 (G)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:09:20.62 +16:16:36.6: 12.31 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:09:20.62 +16:16:36.6: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 09 20.62 +16 16 36.6 11.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3346122743010575616,2461293.9879,11.40,0.05,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 3346122743010575616 20260910.4879 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.27 06:06:28.81 +15:59:06.9
193.61376 -2.36047 galactic Ori Second-epoch detections are separated by 2.0" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.6201+15.9851 | 06:06:28.84 +15:59:06.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.028 (G)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:28.81 +15:59:06.9: 12.25 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:28.81 +15:59:06.9: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 06 28.81 +15 59 06.9 11.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.6201+15.9851,2461293.9879,11.27,0.05,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 J091.6201+15.9851 20260910.4879 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 11.21 06:06:01.22 +15:59:16.3
193.55764 -2.45573 galactic Ori Second-epoch detections are separated by 0.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.5051+15.9878 | 06:06:01.22 +15:59:16.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.341+/-0.030 (G)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:01.22 +15:59:16.3: 12.14 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:01.22 +15:59:16.3: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 06 01.22 +15 59 16.3 11.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.5051+15.9878,2461293.9879,11.21,0.05,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 J091.5051+15.9878 20260910.4879 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4879 2461293.9879 10.90 06:06:22.43 +16:03:22.1
193.53934 -2.34830 galactic Ori Second-epoch detections are separated by 0.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3349004876523579648 | 06:06:22.43 +16:03:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5) J-Ks=0.147+/-0.028 (F)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:22.43 +16:03:22.1: 11.85 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:22.43 +16:03:22.1: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4879* 06 06 22.43 +16 03 22.1 10.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349004876523579648,2461293.9879,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3349004876523579648 20260910.4879 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
First image: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Last image: 2461293.98822593 10.09.2026 11:42:52.720 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
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: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 16779
Objects passed selection criteria: 16644
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 12579.8
Average stars matched: 10851.5 (86.2617 %)
Memory usage VmPeak: 249052 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Sep 10 02:28:55 CDT 2026
VaST build number 1.0rc89-204-g1bee8b93
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 10 06:49:40 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: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
First image: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Last image: 2461293.98822593 10.09.2026 11:42:52.720 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 18 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 129102
Objects passed selection criteria: 128641
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: 101786
Average stars matched: 86403 (84.8871 %)
Memory usage VmPeak: 644244 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Sep 10 02:28:55 CDT 2026
VaST build number 1.0rc89-204-g1bee8b93
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 10 06:50:39 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
SExtractor catalog cache: saved Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461293.98753273
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_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits exists and is non-empty
wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Image size: 941.6'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: 06:13:27.287 +13:59:26.52 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_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits (1st new image)
verification OK: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:13:20.351 +13:59:27.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:20.351 +13:59:27.41
Angular distance between the image centers 0.0280 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits (2nd new image)
verification OK: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:13:23.048 +13:58:57.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:23.048 +13:58:57.33
Angular distance between the image centers 0.0190 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:13:20.351 +13:59:27.41
Second-epoch second image center 06:13:23.048 +13:58:57.33
Angular distance between the image centers 0.01374 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/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.9u693lU74x
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.0eHD8Wbw5v
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits &> /tmp/tmp.E4WRJIdf9H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits &> /tmp/tmp.hYvlZKmqnW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
The reference image (wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits) and catalog (wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat) found
'wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat' -> 'wcsmag.cat'
Read 31404 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6789 deg, Dec +8.6286 to +19.2777 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 85.0776 to 101.6789 deg, Dec 8.6286 to 19.2777 deg
Loaded 17819 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): 13015 out of 14781 total matches.
Matched with Tycho-2 14781 out of 31404 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.949600
a=0.000000 b=1.000000 c=22.949600
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31404 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6789 deg, Dec +8.6286 to +19.2777 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 85.0776 to 101.6789 deg, Dec 8.6286 to 19.2777 deg
Loaded 17819 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): 13015 out of 14781 total matches.
Matched with Tycho-2 14781 out of 31404 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (aperture=6.1)
Read 31324 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 84.9118 to 101.4962 deg, Dec +8.4421 to +19.3403 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 84.9118 to 101.4962 deg, Dec 8.4421 to 19.3403 deg
Loaded 18085 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): 12980 out of 14663 total matches.
Matched with Tycho-2 14663 out of 31324 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -> calib.txt_param_ref_wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (aperture=5.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
2.1 pix Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
2.2 pix fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
2.3 pix fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Limiting magnitude estimates:
15.2 mag. Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
15.2 mag. Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
11.6 mag. fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
11.7 mag. fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 9.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.9u693lU74x (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/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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=3718, bad_region=6433, passed=31404
Got 31404 stars (including 21886 good ones) from the SExtractor catalog wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 31404 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4846 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 4773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 26535 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4845 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 26535 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 26535 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4771 stars left (next iteration limit 5249)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits N_match=4771 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.472 sigma_q2_arcsec=0.364 sigma_q3_arcsec=0.354 sigma_q4_arcsec=0.327 n_q1=1440 n_q2=889 n_q3=1546 n_q4=896 worst_quadrant_to_overall_ratio=1.200
The image catalog is written to wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.0eHD8Wbw5v (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/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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=3619, bad_region=7870, passed=31324
Got 31324 stars (including 20614 good ones) from the SExtractor catalog wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 31324 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4852 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 4780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 24952 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4851 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4779 matched stars entering correct_measured_positions(), 24952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4779 matched stars entering correct_measured_positions(), 24952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4779 stars left (next iteration limit 5258)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits N_match=4779 sigma_overall_arcsec=0.410 sigma_q1_arcsec=0.513 sigma_q2_arcsec=0.384 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.354 n_q1=1323 n_q2=1006 n_q3=1482 n_q4=968 worst_quadrant_to_overall_ratio=1.251
The image catalog is written to wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.E4WRJIdf9H (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.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=189, bad_region=408, passed=1561
Got 1561 stars (including 1009 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat
util/solve_plate_with_UCAC5 got 1561 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.2)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 1197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.2)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 1197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 1197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Excluding outliers - 935 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=935 robust_rms=7.308 arcsec worst_quadrant_rms=10.097 arcsec
SIP_REFIT: SIP order 3 trial: matched=935 robust_rms=0.638 arcsec worst_quadrant_rms=0.703 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=935 robust_rms_before=0.903 arcsec robust_rms_before_corrected=0.908 arcsec robust_rms_after=0.638 arcsec worst_quadrant_rms_before=1.080 worst_quadrant_rms_after=0.703
verification OK: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
verification OK: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:13:20.330 +13:59:26.92 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1561 stars ###
'wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/correct_sextractor_wcs_catalog_usingxy2sky4086005.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 0.903 -> 0.638 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.2 arcsec, 935 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.2)
Done reading UCAC5 zone files...
Matched 865 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 865 pairs (935 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=865 robust_rms=7.022 arcsec worst_quadrant_rms=9.012 arcsec
SIP_REFIT: SIP order 3 trial: matched=865 robust_rms=0.623 arcsec worst_quadrant_rms=0.680 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=865 robust_rms_before=0.623 arcsec robust_rms_before_corrected=0.623 arcsec robust_rms_after=0.623 arcsec worst_quadrant_rms_before=0.680 worst_quadrant_rms_after=0.680
verification OK: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
verification OK: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:13:20.329 +13:59:26.92 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1561 stars ###
'wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/correct_sextractor_wcs_catalog_usingxy2sky4086113.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 0.623 -> 0.623 arcsec)
Accuracy estimation diagnostic: 865 matched stars entering correct_measured_positions(), 1196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 865 matched stars entering correct_measured_positions(), 1180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WCS_QUALITY_DIAG: file=fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits N_match=865 sigma_overall_arcsec=0.629 sigma_q1_arcsec=0.688 sigma_q2_arcsec=0.521 sigma_q3_arcsec=0.659 sigma_q4_arcsec=0.608 n_q1=254 n_q2=205 n_q3=261 n_q4=145 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits -region wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hYvlZKmqnW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.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=215, bad_region=452, passed=1497
Got 1497 stars (including 888 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat
util/solve_plate_with_UCAC5 got 1497 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.2)
Done reading UCAC5 zone files...
Matched 839 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 817 matched stars entering correct_measured_positions(), 801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 817 matched stars entering correct_measured_positions(), 1080 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.2)
Done reading UCAC5 zone files...
Matched 839 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 816 matched stars entering correct_measured_positions(), 1081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 816 matched stars entering correct_measured_positions(), 1081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 816 stars left (next iteration limit 898)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=816 robust_rms=8.058 arcsec worst_quadrant_rms=10.676 arcsec
SIP_REFIT: SIP order 3 trial: matched=816 robust_rms=0.644 arcsec worst_quadrant_rms=0.827 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=816 robust_rms_before=0.965 arcsec robust_rms_before_corrected=0.738 arcsec robust_rms_after=0.644 arcsec worst_quadrant_rms_before=0.899 worst_quadrant_rms_after=0.827
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.899 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits N_match=816 sigma_overall_arcsec=0.774 sigma_q1_arcsec=0.711 sigma_q2_arcsec=0.925 sigma_q3_arcsec=0.778 sigma_q4_arcsec=0.662 n_q1=154 n_q2=233 n_q3=250 n_q4=179 worst_quadrant_to_overall_ratio=1.195
The image catalog is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits -region wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits to local_wcs_cache/
'wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'local_wcs_cache/wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits'
Saving the final (post-refit) wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits'
Saving the final (post-refit) wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits'
Saving the final (post-refit) wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits sigma_overall=0.393 worst_q_ratio=1.200
ref2=Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits sigma_overall=0.410 worst_q_ratio=1.251
new1=fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits sigma_overall=0.629 worst_q_ratio=1.094
new2=fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits sigma_overall=0.774 worst_q_ratio=1.195
reference average sigma_overall=0.4015 worst_q_ratio=1.2255
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386_astrometric_residuals.png (4771 matched stars from wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042_astrometric_residuals.png (4779 matched stars from wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166_astrometric_residuals.png (865 matched stars from wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167_astrometric_residuals.png (816 matched stars from wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.72 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits'
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits'
Preparing the HTML report for the field Ori-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ori-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
SExtractor catalog cache: saved Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Creating symlink local_wcs_cache/wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits exists and is non-empty
wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Image size: 941.6'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: 06:13:27.287 +13:59:26.52 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_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits (1st new image)
verification OK: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:13:20.329 +13:59:26.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:20.329 +13:59:26.92
Angular distance between the image centers 0.0281 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits (2nd new image)
verification OK: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:13:23.048 +13:58:57.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:23.048 +13:58:57.33
Angular distance between the image centers 0.0190 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:13:20.329 +13:59:26.92
Second-epoch second image center 06:13:23.048 +13:58:57.33
Angular distance between the image centers 0.01373 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/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.xzKPAgCgDl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.9vgq02HcEP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits &> /tmp/tmp.Bff0ON0Q3Q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits &> /tmp/tmp.hzrWLbxrjj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
The reference image (wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits) and catalog (wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat) found
'wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat' -> 'wcsmag.cat'
Read 229058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6828 deg, Dec +8.6174 to +19.2791 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 85.0776 to 101.6828 deg, Dec 8.6174 to 19.2791 deg
Loaded 17847 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): 9852 out of 15551 total matches.
Matched with Tycho-2 15551 out of 229058 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.805100
a=0.000000 b=1.000000 c=22.805100
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 229058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6828 deg, Dec +8.6174 to +19.2791 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 85.0776 to 101.6828 deg, Dec 8.6174 to 19.2791 deg
Loaded 17847 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): 9852 out of 15551 total matches.
Matched with Tycho-2 15551 out of 229058 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (aperture=4.6)
Read 230307 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 84.9070 to 101.4968 deg, Dec +8.4421 to +19.3422 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 84.9070 to 101.4968 deg, Dec 8.4421 to 19.3422 deg
Loaded 18095 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): 10167 out of 15481 total matches.
Matched with Tycho-2 15481 out of 230307 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -> calib.txt_param_ref_wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
1.9 pix Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
2.0 pix fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
2.0 pix fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Limiting magnitude estimates:
15.4 mag. Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
15.5 mag. Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
12.0 mag. fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
12.1 mag. fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
All-image limiting magnitude estimate: 12.0 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xzKPAgCgDl (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/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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=66, blended=37651, bad_region=39353, passed=228992
Got 228992 stars (including 156979 good ones) from the SExtractor catalog wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 228992 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4829 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 4781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 199193 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4828 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 199193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 199192 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4780 stars left (next iteration limit 5259)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits N_match=4780 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.337 n_q1=1420 n_q2=868 n_q3=1591 n_q4=901 worst_quadrant_to_overall_ratio=1.162
The image catalog is written to wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.9vgq02HcEP (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/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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=51, blended=35229, bad_region=43140, passed=230256
Got 230256 stars (including 157786 good ones) from the SExtractor catalog wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 230256 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4828 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4775 matched stars entering correct_measured_positions(), 4775 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4775 matched stars entering correct_measured_positions(), 195841 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4827 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4773 matched stars entering correct_measured_positions(), 195841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4773 matched stars entering correct_measured_positions(), 195841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4773 stars left (next iteration limit 5252)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits N_match=4773 sigma_overall_arcsec=0.402 sigma_q1_arcsec=0.509 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.376 sigma_q4_arcsec=0.326 n_q1=1383 n_q2=982 n_q3=1493 n_q4=915 worst_quadrant_to_overall_ratio=1.264
The image catalog is written to wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Bff0ON0Q3Q (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.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=1, no_mag_err=0, low_SNR=2, blended=600, bad_region=4226, passed=20770
Got 20770 stars (including 16053 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat
util/solve_plate_with_UCAC5 got 20770 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4830 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4742 matched stars entering correct_measured_positions(), 4745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4742 matched stars entering correct_measured_positions(), 17629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4830 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4741 matched stars entering correct_measured_positions(), 17629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 4741 matched stars entering correct_measured_positions(), 17629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 4741 stars left (next iteration limit 5216)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4741 robust_rms=7.095 arcsec worst_quadrant_rms=8.989 arcsec
SIP_REFIT: SIP order 3 trial: matched=4741 robust_rms=0.672 arcsec worst_quadrant_rms=0.784 arcsec
SIP_REFIT: SIP order 5 trial: matched=4741 robust_rms=0.583 arcsec worst_quadrant_rms=0.655 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4741 robust_rms_before=0.688 arcsec robust_rms_before_corrected=0.642 arcsec robust_rms_after=0.583 arcsec worst_quadrant_rms_before=0.696 worst_quadrant_rms_after=0.655
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.696 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits N_match=4741 sigma_overall_arcsec=0.668 sigma_q1_arcsec=0.642 sigma_q2_arcsec=0.666 sigma_q3_arcsec=0.731 sigma_q4_arcsec=0.608 n_q1=1427 n_q2=1083 n_q3=1354 n_q4=877 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits -region wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hzrWLbxrjj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.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=591, bad_region=4078, passed=19920
Got 19920 stars (including 15378 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat
util/solve_plate_with_UCAC5 got 19920 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4769 matched stars entering correct_measured_positions(), 4770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4768 matched stars entering correct_measured_positions(), 16891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4767 matched stars entering correct_measured_positions(), 16891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 4767 matched stars entering correct_measured_positions(), 16891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 4767 stars left (next iteration limit 5244)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4767 robust_rms=7.218 arcsec worst_quadrant_rms=8.170 arcsec
SIP_REFIT: SIP order 3 trial: matched=4767 robust_rms=0.671 arcsec worst_quadrant_rms=0.813 arcsec
SIP_REFIT: SIP order 5 trial: matched=4767 robust_rms=0.601 arcsec worst_quadrant_rms=0.652 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4767 robust_rms_before=0.947 arcsec robust_rms_before_corrected=0.663 arcsec robust_rms_after=0.601 arcsec worst_quadrant_rms_before=0.727 worst_quadrant_rms_after=0.652
SIP_REFIT: applied the refit solution to the output catalog positions only (order 5, robust RMS 0.947 -> 0.601 arcsec); the image header was NOT rewritten as wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits is a symbolic link
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4767 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4572 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4572 pairs (4767 from the initial matching)
SIP_REFIT: wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4572 robust_rms=6.962 arcsec worst_quadrant_rms=7.779 arcsec
SIP_REFIT: SIP order 3 trial: matched=4572 robust_rms=0.658 arcsec worst_quadrant_rms=0.787 arcsec
SIP_REFIT: SIP order 5 trial: matched=4572 robust_rms=0.590 arcsec worst_quadrant_rms=0.648 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4572 robust_rms_before=0.590 arcsec robust_rms_before_corrected=0.590 arcsec robust_rms_after=0.590 arcsec worst_quadrant_rms_before=0.646 worst_quadrant_rms_after=0.648
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.648 vs 0.646 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 4572 matched stars entering correct_measured_positions(), 16891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 4572 matched stars entering correct_measured_positions(), 16889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
WCS_QUALITY_DIAG: file=fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits N_match=4572 sigma_overall_arcsec=0.615 sigma_q1_arcsec=0.628 sigma_q2_arcsec=0.589 sigma_q3_arcsec=0.690 sigma_q4_arcsec=0.571 n_q1=1017 n_q2=1288 n_q3=1248 n_q4=1019 worst_quadrant_to_overall_ratio=1.123
The image catalog is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits -region wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-41-52_20.00sec_-0.00C_LIGHT_0166.fits
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q2b1x1_064725_TTUQ2b1x1_4076832_lvABsMU2/wcs_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167.fits
Preparing the HTML report for the field Ori-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:46:08.30 +10:26:38.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:53:47.39 +12:36:33.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:46:38.15 +10:29:11.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:08:09.05 +16:24:31.6: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:24.19 +11:14:16.6: 12.81 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:09:55.06 +16:35:39.8: 12.11 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:07:01.43 +16:16:38.4: 12.96 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:46:38.15 +10:29:11.1: 12.45 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:46:08.30 +10:26:38.1: 12.58 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:53:47.39 +12:36:33.2: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Forced photometry filter KEPT candidate at 05:46:38.15 +10:29:11.1: ref_mag=12.45 +/- 0.01 new_mean_mag=11.3448 delta=1.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter KEPT candidate at 05:46:08.30 +10:26:38.1: ref_mag=12.58 +/- 0.02 new_mean_mag=11.4786 delta=1.11 (need > 0.90)
Forced photometry filter KEPT candidate at 05:53:47.39 +12:36:33.2: ref_mag=12.66 +/- 0.02 new_mean_mag=11.5969 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:08:09.05 +16:24:31.6: 12.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 06:08:09.05 +16:24:31.6: ref_mag=12.75 +/- 0.01 new_mean_mag=11.6506 delta=1.10 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:24.19 +11:14:16.6: 12.81 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:07:01.43 +16:16:38.4: 12.95 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:09:55.06 +16:35:39.8: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:24.19 +11:14:16.6: ref_mag=12.81 +/- 0.01 new_mean_mag=11.7346 delta=1.07 (need > 0.90)
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter KEPT candidate at 06:07:01.43 +16:16:38.4: ref_mag=12.96 +/- 0.01 new_mean_mag=11.7579 delta=1.20 (need > 0.90)
Forced photometry filter KEPT candidate at 06:09:55.06 +16:35:39.8: ref_mag=12.10 +/- 0.01 new_mean_mag=11.0879 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:28.28 +17:55:33.4: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:05:44.58 +15:59:44.1: 12.76 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:51.25 +16:02:04.1: 12.69 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:28.28 +17:55:33.4: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 06:20:28.28 +17:55:33.4: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7689 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:05:44.58 +15:59:44.1: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 06:05:44.58 +15:59:44.1: ref_mag=12.77 +/- 0.01 new_mean_mag=11.6182 delta=1.15 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:51.25 +16:02:04.1: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 06:06:51.25 +16:02:04.1: ref_mag=12.67 +/- 0.01 new_mean_mag=11.5930 delta=1.08 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:45:53.45 +10:19:05.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:31.55 +11:13:54.5: 12.65 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:08:46.97 +16:33:36.5: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:45:53.45 +10:19:05.8: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Forced photometry filter KEPT candidate at 05:45:53.45 +10:19:05.8: ref_mag=11.60 +/- 0.01 new_mean_mag=10.5615 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:31.55 +11:13:54.5: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:31.55 +11:13:54.5: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6006 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:08:46.97 +16:33:36.5: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 06:08:46.97 +16:33:36.5: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6301 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:07:08.35 +16:15:19.9: 12.62 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:07:08.35 +16:15:19.9: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 06:07:08.35 +16:15:19.9: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6076 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:22.32 +16:01:33.9: 12.60 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:09:43.53 +16:47:47.2: 12.56 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:22.32 +16:01:33.9: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 06:06:22.32 +16:01:33.9: ref_mag=12.60 +/- 0.01 new_mean_mag=11.4055 delta=1.19 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:09:43.53 +16:47:47.2: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 06:09:43.53 +16:47:47.2: ref_mag=12.56 +/- 0.01 new_mean_mag=11.5709 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:44.69 +15:57:55.3: 12.55 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:44.69 +15:57:55.3: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 06:06:44.69 +15:57:55.3: ref_mag=12.52 +/- 0.01 new_mean_mag=11.4705 delta=1.05 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:12.32 +16:00:13.0: 12.45 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:08:50.34 +16:42:28.8: 12.16 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:12.32 +16:00:13.0: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 06:06:12.32 +16:00:13.0: ref_mag=12.43 +/- 0.01 new_mean_mag=11.4744 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:08:50.34 +16:42:28.8: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter REJECTED candidate at 06:08:50.34 +16:42:28.8: ref_mag=12.11 +/- 0.01 new_mean_mag=11.2212 delta=0.89 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:09:20.62 +16:16:36.6: 12.31 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:28.81 +15:59:06.9: 12.25 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:09:20.62 +16:16:36.6: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 06:09:20.62 +16:16:36.6: ref_mag=12.31 +/- 0.01 new_mean_mag=11.3617 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:28.81 +15:59:06.9: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter KEPT candidate at 06:06:28.81 +15:59:06.9: ref_mag=12.24 +/- 0.01 new_mean_mag=11.2650 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:01.22 +15:59:16.3: 12.14 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:01.22 +15:59:16.3: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter KEPT candidate at 06:06:01.22 +15:59:16.3: ref_mag=12.14 +/- 0.01 new_mean_mag=11.2140 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q2b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:06:22.43 +16:03:22.1: 11.85 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q2b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:06:22.43 +16:03:22.1: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.00
Forced photometry filter KEPT candidate at 06:06:22.43 +16:03:22.1: ref_mag=11.83 +/- 0.00 new_mean_mag=10.8815 delta=0.95 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out244937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out178044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69707.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 26s
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: 7s
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Considering the candidate 56128_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 56128_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 184758_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
The candidate 184758_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167 did not pass the final checks
**** FOUND 06:26:52.72 +10:23:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62677_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 62677_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 21204_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
The candidate 21204_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167 did not pass the final checks
**** FOUND 06:19:43.63 +18:15:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248883_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
The candidate 248883_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167 did not pass the final checks
**** FOUND 05:53:47.39 +12:36:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 1.047 3343300090504153600 088.44750828852 +12.60893544133 12.3421 11.5474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248513_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
The candidate 248513_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167 did not pass the final checks
**** FOUND 05:46:08.30 +10:26:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 0.835 3336893446705046912 086.53438434454 +10.44404103246 12.3957 11.7251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248237_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
The candidate 248237_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167 did not pass the final checks
**** FOUND 05:46:18.61 +10:19:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178044_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 178044_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 247819_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
The candidate 247819_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167 did not pass the final checks
**** FOUND 05:46:38.15 +10:29:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 0.525 3336896813959551104 086.65900025475 +10.48655651864 12.1822 11.4669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 59922_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 59922_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 27729_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 27729_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 68922_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 68922_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 67987_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 67987_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 178280_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 178280_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 244937_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
The candidate 244937_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167 did not pass the final checks
**** FOUND 05:45:53.45 +10:19:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 0.541 3336887811708001792 086.47256466576 +10.31822700604 11.2829 10.5033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56654_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 56654_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 63146_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 63146_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 68272_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 68272_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 51627_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 51627_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 69707_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 69707_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 68769_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
Preparing report for the candidate 68769_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
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Considering the candidate 53317_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167
The candidate 53317_fd_Ori-02-Q2b1x1_2026-09-10_06-42-52_20.00sec_-0.00C_LIGHT_0167 did not pass the final checks
