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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl
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 10.4844 2461293.9844 12.31 05:44:33.03 +14:56:53.2
191.87069 -7.45738 galactic Tau Second-epoch detections are separated by 3.3" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.59 Elpis -0 0 1 13.1 -0 0
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:44:33.03 +14:56:53.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:44:33.03 +14:56:53.2: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 44 33.03 +14 56 53.2 12.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461293.9844,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260910.4844 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 10.99 06:34:30.89 +13:22:15.7
199.11919 2.38253 galactic Gem Second-epoch detections are separated by 0.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3355418907668074240 | 06:34:30.93 +13:22:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.470+/-0.032 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:30.89 +13:22:15.7: 11.84 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:30.89 +13:22:15.7: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3355418907668074240,2461293.9844,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3355418907668074240 20260910.4844 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 11.23 06:34:14.71 +13:23:20.8
199.07296 2.33257 galactic Gem Second-epoch detections are separated by 1.6" and 8.8 pix
The object was found in VSX 1" Gaia DR3 3355606791014664320
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.050 G 12.080 G F
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:14.71 +13:23:20.8: 12.15 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:14.71 +13:23:20.8: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3355606791014664320,2461293.9844,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3355606791014664320 20260910.4844 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 11.35 06:34:36.57 +13:54:59.3
198.64469 2.65332 galactic Gem Second-epoch detections are separated by 2.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3355663931259083776 | 06:34:36.53 +13:54:59.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A2V (LAMOST DR5) J-Ks=0.230+/-0.031 (F)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:36.57 +13:54:59.3: 12.26 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:36.57 +13:54:59.3: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3355663931259083776,2461293.9844,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3355663931259083776 20260910.4844 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 11.70 06:34:33.48 +13:31:10.2
198.99199 2.46002 galactic Gem Second-epoch detections are separated by 1.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3355614552015690752 | 06:34:33.45 +13:31:10.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.816+/-0.033 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:33.48 +13:31:10.2: 12.73 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:33.48 +13:31:10.2: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3355614552015690752,2461293.9844,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3355614552015690752 20260910.4844 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 11.88 05:43:47.76 +14:35:55.4
192.07963 -7.79272 galactic Tau Second-epoch detections are separated by 0.3" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:43:47.76 +14:35:55.4 (user input) | T | P | (position from user input) J-Ks=0.737+/-0.026 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:47.76 +14:35:55.4: 12.74 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:47.76 +14:35:55.4: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 10.4844* 05 43 47.76 +14 35 55.4 11.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9844,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4844 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 12.04 05:42:55.06 +13:34:38.6
192.85671 -8.49753 galactic Ori Second-epoch detections are separated by 0.9" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:42:55.06 +13:34:38.6 (user input) | T | P | (position from user input) J-Ks=0.866+/- (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:42:55.06 +13:34:38.6: 12.93 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:42:55.06 +13:34:38.6: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 42 55.06 +13 34 38.6 12.0 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,2461293.9844,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4844 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 12.11 05:43:47.25 +14:10:05.8
192.45216 -8.01438 galactic Tau Second-epoch detections are separated by 1.8" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.9467+14.1681 | 05:43:47.22 +14:10:05.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.410+/-0.054 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:47.25 +14:10:05.8: 13.09 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:47.25 +14:10:05.8: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 43 47.25 +14 10 05.8 12.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.9467+14.1681,2461293.9844,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.9467+14.1681 20260910.4844 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.4844 2461293.9844 12.06 05:57:29.11 +15:42:53.0
192.78451 -4.37729 galactic Ori Second-epoch detections are separated by 4.8" and 9.6 pix
The object was found in VSX 8" Gaia DR3 3348766248138047872
Type: E
# Max. Min./Amp. JD0 Period
18.350 G 18.740 G 0.285443000000
ATTENTION: measured mag 12.06 is 6.3 mag brighter than the VSX record maximum brightness 18.35 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:57:29.11 +15:42:53.0: 13.06 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:57:29.11 +15:42:53.0: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 57 29.11 +15 42 53.0 12.1 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 3348766248138047872,2461293.9844,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3348766248138047872 20260910.4844 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.4844 2461293.9844 12.13 05:43:37.50 +14:16:13.0
192.34329 -7.99615 galactic Tau Second-epoch detections are separated by 0.9" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:43:37.50 +14:16:13.0 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.028 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:37.50 +14:16:13.0: 13.11 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:37.50 +14:16:13.0: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 43 37.50 +14 16 13.0 12.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9844,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4844 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 12.04 06:00:54.72 +14:40:24.2
194.10202 -4.17310 galactic Ori Second-epoch detections are separated by 1.5" and 9.2 pix
The object was found in VSX 1" Gaia DR3 3345433250439433088
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.000 G 13.030 G A
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:00:54.72 +14:40:24.2: 13.11 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:00:54.72 +14:40:24.2: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 06 00 54.72 +14 40 24.2 12.0 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 3345433250439433088,2461293.9844,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3345433250439433088 20260910.4844 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 12.15 05:49:37.58 +17:24:20.6
190.36810 -5.15638 galactic Tau Second-epoch detections are separated by 2.6" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:49:37.58 +17:24:20.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.515+/-0.028 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:49:37.58 +17:24:20.6: 13.08 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:49:37.58 +17:24:20.6: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 49 37.58 +17 24 20.6 12.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9844,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4844 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 12.10 05:49:11.49 +17:39:47.2
190.09266 -5.11475 galactic Tau Second-epoch detections are separated by 1.6" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:49:11.49 +17:39:47.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.303+/-0.028 (F)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:49:11.49 +17:39:47.2: 13.06 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:49:11.49 +17:39:47.2: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 49 11.49 +17 39 47.2 12.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9844,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4844 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 12.06 06:00:03.13 +14:47:30.9
193.89596 -4.29571 galactic Ori Second-epoch detections are separated by 3.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.0127+14.7891 | 06:00:03.13 +14:47:30.9 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.402+/-0.028 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:00:03.13 +14:47:30.9: 13.05 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:00:03.13 +14:47:30.9: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 06 00 03.13 +14 47 30.9 12.1 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 J090.0127+14.7891,2461293.9844,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.0127+14.7891 20260910.4844 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.4844 2461293.9844 12.02 05:43:37.50 +14:23:14.3
192.24171 -7.93636 galactic Tau Second-epoch detections are separated by 3.7" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.8955+14.3930 | 05:43:37.50 +14:23:14.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.168+/-0.033 (F)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:37.50 +14:23:14.3: 13.05 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:37.50 +14:23:14.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 43 37.50 +14 23 14.3 12.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.8955+14.3930,2461293.9844,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.8955+14.3930 20260910.4844 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 12.09 05:43:34.93 +14:23:46.5
192.22860 -7.94070 galactic Tau Second-epoch detections are separated by 0.7" and 9.2 pix
The object was found in VSX 1" ASASSN-V J054334.90+142345.1
Type: SR
# Max. Min./Amp. JD0 Period
14.350 g Y 0.270 g 2459443.09200 393.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:34.93 +14:23:46.5: 13.01 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:34.93 +14:23:46.5: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 43 34.93 +14 23 46.5 12.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054334.90+142345.1,2461293.9844,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J054334.90+142345.1 20260910.4844 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 12.04 05:50:10.50 +17:38:30.8
190.23056 -4.92376 galactic Tau Second-epoch detections are separated by 0.8" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:50:10.50 +17:38:30.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.668+/-0.028 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:50:10.50 +17:38:30.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:50:10.50 +17:38:30.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 50 10.50 +17 38 30.8 12.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9844,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4844 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 11.88 05:43:13.18 +14:04:44.0
192.45876 -8.17839 galactic Tau Second-epoch detections are separated by 0.6" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:43:13.18 +14:04:44.0 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.026 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:13.18 +14:04:44.0: 12.83 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:13.18 +14:04:44.0: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 43 13.18 +14 04 44.0 11.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9844,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4844 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 11.91 05:42:48.30 +13:50:55.6
192.60670 -8.38246 galactic Ori Second-epoch detections are separated by 2.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:42:48.30 +13:50:55.6 (user input) | T | P | (position from user input) J-Ks=0.527+/-0.028 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:42:48.30 +13:50:55.6: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:42:48.30 +13:50:55.6: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4844* 05 42 48.30 +13 50 55.6 11.9 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
target,2461293.9844,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4844 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 11.80 05:44:14.46 +14:39:59.5
192.07633 -7.66554 galactic Tau Second-epoch detections are separated by 2.0" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3347544171027504768 | 05:44:12.67 +14:39:55.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.693+/-0.028 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:44:14.46 +14:39:59.5: 12.58 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:44:14.46 +14:39:59.5: 12.68 +/- 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 10.4844* 05 44 14.46 +14 39 59.5 11.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3347544171027504768,2461293.9844,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3347544171027504768 20260910.4844 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 11.31 06:34:33.18 +13:29:53.2
199.01046 2.44912 galactic Gem Second-epoch detections are separated by 0.8" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3355613761741709056 | 06:34:33.16 +13:29:52.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.262+/-0.033 (F)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:33.18 +13:29:53.2: 12.38 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:33.18 +13:29:53.2: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3355613761741709056,2461293.9844,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3355613761741709056 20260910.4844 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4844 2461293.9844 11.26 06:33:53.80 +13:29:54.3
198.93683 2.30754 galactic Gem Second-epoch detections are separated by 0.9" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3355611567018005632 | 06:33:53.85 +13:29:53.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.031 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:33:53.80 +13:29:54.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:33:53.80 +13:29:54.3: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3355611567018005632,2461293.9844,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3355611567018005632 20260910.4844 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.4844 2461293.9844 11.40 06:33:48.25 +13:26:59.1
198.96974 2.26520 galactic Gem Second-epoch detections are separated by 1.3" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3355610776744319872 | 06:33:48.28 +13:26:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.689+/-0.029 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:33:48.25 +13:26:59.1: 12.27 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:33:48.25 +13:26:59.1: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3355610776744319872,2461293.9844,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3355610776744319872 20260910.4844 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 10.4844 2461293.9844 10.86 06:34:00.94 +13:36:34.1
198.85141 2.38426 galactic Gem Second-epoch detections are separated by 1.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3355619156220629376 | 06:34:00.96 +13:36:33.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.242+/-0.027 (F)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:00.94 +13:36:34.1: 11.78 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:00.94 +13:36:34.1: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3355619156220629376,2461293.9844,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3355619156220629376 20260910.4844 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Last image: 2461293.98471958 10.09.2026 11:37:49.772 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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): 27959
Objects passed selection criteria: 27775
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: 16470.2
Average stars matched: 15635.2 (94.9303 %)
Memory usage VmPeak: 253092 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Sep 10 02:28:55 CDT 2026
VaST build number 1.0rc89-204-g1bee8b93
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 10 06:39:47 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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Last image: 2461293.98471958 10.09.2026 11:37:49.772 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 42
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 33 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): 202760
Objects passed selection criteria: 202059
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: 123139
Average stars matched: 116172 (94.3428 %)
Memory usage VmPeak: 602208 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 06:41:12 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
SExtractor catalog cache: saved Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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: 2461293.98406977
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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Ori-02-Q1b1x1_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-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits (1st new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:28.237 +13:59:28.91 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 06:13:28.237 +13:59:28.91
Angular distance between the image centers 0.0039 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits (2nd new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:25.389 +14:00:02.33 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 06:13:25.389 +14:00:02.33
Angular distance between the image centers 0.0126 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 06:13:28.237 +13:59:28.91
Second-epoch second image center 06:13:25.389 +14:00:02.33
Angular distance between the image centers 0.01479 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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.7LVHi3lzMP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.GHUkEi3r55
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits &> /tmp/tmp.T9iTCEq5jN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits &> /tmp/tmp.bClKnvLTrT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
The reference image (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits) and catalog (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat) found
'wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (aperture=5.9)
____ 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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
2.1 pix Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
2.7 pix fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
2.8 pix fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Limiting magnitude estimates:
15.2 mag. Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
15.2 mag. Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
11.8 mag. fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
12.1 mag. fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
All-image limiting magnitude estimate: 11.8 (SNR ) 9.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.7LVHi3lzMP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'wcs_Ori-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3718, bad_region=0, passed=31404
Got 31404 stars (including 27641 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_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 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: 4785 matched stars entering correct_measured_positions(), 4786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4785 matched stars entering correct_measured_positions(), 31404 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 4848 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 31404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 31404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4783 stars left (next iteration limit 5263)
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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits N_match=4783 sigma_overall_arcsec=0.380 sigma_q1_arcsec=0.478 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.323 n_q1=1170 n_q2=1223 n_q3=1237 n_q4=1153 worst_quadrant_to_overall_ratio=1.257
The image catalog is written to wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_Ori-02-Q1b1x1_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-Q1b1x1_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.GHUkEi3r55 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Ori-02-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3619, bad_region=0, passed=31324
Got 31324 stars (including 27657 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_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 4850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4788 matched stars entering correct_measured_positions(), 4788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4788 matched stars entering correct_measured_positions(), 31324 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 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4788 matched stars entering correct_measured_positions(), 31324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4787 matched stars entering correct_measured_positions(), 31324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4787 stars left (next iteration limit 5266)
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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits N_match=4787 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.498 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.371 sigma_q4_arcsec=0.355 n_q1=1017 n_q2=1324 n_q3=1130 n_q4=1316 worst_quadrant_to_overall_ratio=1.226
The image catalog is written to wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Ori-02-Q1b1x1_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-Q1b1x1_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.T9iTCEq5jN (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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=98, bad_region=0, passed=1628
Got 1628 stars (including 1530 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat
util/solve_plate_with_UCAC5 got 1628 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.5)
Done reading UCAC5 zone files...
Matched 1450 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1419 matched stars entering correct_measured_positions(), 1388 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1419 matched stars entering correct_measured_positions(), 1589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 549 (Dec 8.5 to 19.5)
Done reading UCAC5 zone files...
Matched 1452 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1420 matched stars entering correct_measured_positions(), 1594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 1420 matched stars entering correct_measured_positions(), 1591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 1420 stars left (next iteration limit 1560)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1420 robust_rms=7.696 arcsec worst_quadrant_rms=47.725 arcsec
SIP_REFIT: SIP order 3 trial: matched=1420 robust_rms=0.414 arcsec worst_quadrant_rms=0.605 arcsec
SIP_REFIT: SIP order 5 trial: matched=1420 robust_rms=0.325 arcsec worst_quadrant_rms=0.500 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1420 robust_rms_before=0.895 arcsec robust_rms_before_corrected=0.518 arcsec robust_rms_after=0.325 arcsec worst_quadrant_rms_before=0.702 worst_quadrant_rms_after=0.500
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:28.235 +13:59:28.21 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1628 stars ###
'wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/correct_sextractor_wcs_catalog_usingxy2sky3794269.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.895 -> 0.325 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 1420 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 549 (Dec 8.5 to 19.5)
Done reading UCAC5 zone files...
Matched 1341 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 1341 pairs (1420 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=1341 robust_rms=7.107 arcsec worst_quadrant_rms=51.888 arcsec
SIP_REFIT: SIP order 3 trial: matched=1341 robust_rms=0.407 arcsec worst_quadrant_rms=0.568 arcsec
SIP_REFIT: SIP order 5 trial: matched=1341 robust_rms=0.314 arcsec worst_quadrant_rms=0.427 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1341 robust_rms_before=0.317 arcsec robust_rms_before_corrected=0.317 arcsec robust_rms_after=0.314 arcsec worst_quadrant_rms_before=0.435 worst_quadrant_rms_after=0.427
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:28.235 +13:59:28.21 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1628 stars ###
'wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/correct_sextractor_wcs_catalog_usingxy2sky3803301.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.317 -> 0.314 arcsec)
Accuracy estimation diagnostic: 1341 matched stars entering correct_measured_positions(), 1586 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 1341 matched stars entering correct_measured_positions(), 1582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits N_match=1341 sigma_overall_arcsec=0.332 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.455 sigma_q3_arcsec=0.295 sigma_q4_arcsec=0.413 n_q1=336 n_q2=138 n_q3=687 n_q4=180 worst_quadrant_to_overall_ratio=1.368
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits -region wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.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.bClKnvLTrT (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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=137, bad_region=0, passed=1965
Got 1965 stars (including 1828 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat
util/solve_plate_with_UCAC5 got 1965 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.5)
Done reading UCAC5 zone files...
Matched 1757 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1721 matched stars entering correct_measured_positions(), 1695 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1720 matched stars entering correct_measured_positions(), 1929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 549 (Dec 8.5 to 19.5)
Done reading UCAC5 zone files...
Matched 1758 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1718 matched stars entering correct_measured_positions(), 1932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 1718 matched stars entering correct_measured_positions(), 1931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 1718 stars left (next iteration limit 1892)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1718 robust_rms=9.081 arcsec worst_quadrant_rms=20.926 arcsec
SIP_REFIT: SIP order 3 trial: matched=1718 robust_rms=0.406 arcsec worst_quadrant_rms=0.498 arcsec
SIP_REFIT: SIP order 5 trial: matched=1718 robust_rms=0.339 arcsec worst_quadrant_rms=0.495 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1718 robust_rms_before=0.814 arcsec robust_rms_before_corrected=0.495 arcsec robust_rms_after=0.406 arcsec worst_quadrant_rms_before=0.665 worst_quadrant_rms_after=0.498
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:25.384 +14:00:01.69 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1965 stars ###
'wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/correct_sextractor_wcs_catalog_usingxy2sky3794161.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 0.814 -> 0.406 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 1718 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 549 (Dec 8.5 to 19.5)
Done reading UCAC5 zone files...
Matched 1588 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 1588 pairs (1718 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=1588 robust_rms=8.360 arcsec worst_quadrant_rms=19.948 arcsec
SIP_REFIT: SIP order 3 trial: matched=1588 robust_rms=0.394 arcsec worst_quadrant_rms=0.489 arcsec
SIP_REFIT: SIP order 5 trial: matched=1588 robust_rms=0.332 arcsec worst_quadrant_rms=0.462 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1588 robust_rms_before=0.395 arcsec robust_rms_before_corrected=0.395 arcsec robust_rms_after=0.332 arcsec worst_quadrant_rms_before=0.489 worst_quadrant_rms_after=0.462
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:25.389 +14:00:01.55 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1965 stars ###
'wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/correct_sextractor_wcs_catalog_usingxy2sky3803280.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.395 -> 0.332 arcsec)
Accuracy estimation diagnostic: 1588 matched stars entering correct_measured_positions(), 1920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 1588 matched stars entering correct_measured_positions(), 1915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits N_match=1588 sigma_overall_arcsec=0.351 sigma_q1_arcsec=0.377 sigma_q2_arcsec=0.425 sigma_q3_arcsec=0.295 sigma_q4_arcsec=0.422 n_q1=505 n_q2=208 n_q3=657 n_q4=218 worst_quadrant_to_overall_ratio=1.211
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits -region wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits to local_wcs_cache/
'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'local_wcs_cache/wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits'
Saving the final (post-refit) wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits'
Saving the final (post-refit) wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits'
Saving the final (post-refit) wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits sigma_overall=0.380 worst_q_ratio=1.257
ref2=Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits sigma_overall=0.407 worst_q_ratio=1.226
new1=fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits sigma_overall=0.332 worst_q_ratio=1.368
new2=fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits sigma_overall=0.351 worst_q_ratio=1.211
reference average sigma_overall=0.3935 worst_q_ratio=1.2415
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386_astrometric_residuals.png (4783 matched stars from wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042_astrometric_residuals.png (4787 matched stars from wcs_Ori-02-Q1b1x1_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-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095_astrometric_residuals.png (1341 matched stars from wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096_astrometric_residuals.png (1588 matched stars from wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits'
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits'
Preparing the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
SExtractor catalog cache: saved Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Creating symlink local_wcs_cache/wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Ori-02-Q1b1x1_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-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits (1st new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:28.235 +13:59:28.21 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 06:13:28.235 +13:59:28.21
Angular distance between the image centers 0.0039 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits (2nd new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:25.389 +14:00:01.55 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 06:13:25.389 +14:00:01.55
Angular distance between the image centers 0.0124 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 06:13:28.235 +13:59:28.21
Second-epoch second image center 06:13:25.389 +14:00:01.55
Angular distance between the image centers 0.01477 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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.rsW3zICw3o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.OlI5sWp10q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits &> /tmp/tmp.IxnQOh6YAL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits &> /tmp/tmp.IbfUWBA2Iq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
The reference image (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits) and catalog (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat) found
'wcs_Ori-02-Q1b1x1_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.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 36 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
1.9 pix Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
2.6 pix fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
2.6 pix fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Limiting magnitude estimates:
15.4 mag. Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
15.4 mag. Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
12.5 mag. fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
12.6 mag. fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rsW3zICw3o (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'wcs_Ori-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=66, blended=37651, bad_region=12, passed=228992
Got 228992 stars (including 190970 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_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 4823 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 228992 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 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 228992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 228992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4770 stars left (next iteration limit 5249)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits N_match=4770 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.454 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.325 n_q1=1096 n_q2=1242 n_q3=1241 n_q4=1191 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_Ori-02-Q1b1x1_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-Q1b1x1_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.OlI5sWp10q (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Ori-02-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=82, blended=35229, bad_region=4, passed=230225
Got 230225 stars (including 194609 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 230225 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 4832 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(), 230225 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 4831 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 230225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 230225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4778 stars left (next iteration limit 5259)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits N_match=4778 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.356 sigma_q4_arcsec=0.328 n_q1=1035 n_q2=1329 n_q3=1162 n_q4=1252 worst_quadrant_to_overall_ratio=1.248
The image catalog is written to wcs_Ori-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Ori-02-Q1b1x1_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-Q1b1x1_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.IxnQOh6YAL (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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=405, bad_region=0, passed=16458
Got 16458 stars (including 16027 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat
util/solve_plate_with_UCAC5 got 16458 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.4 to 19.5)
Done reading UCAC5 zone files...
Matched 4814 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4730 matched stars entering correct_measured_positions(), 4730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4730 matched stars entering correct_measured_positions(), 16451 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 549 (Dec 8.4 to 19.5)
Done reading UCAC5 zone files...
Matched 4815 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4727 matched stars entering correct_measured_positions(), 16452 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4727 matched stars entering correct_measured_positions(), 16452 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 4727 stars left (next iteration limit 5203)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.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=4727 robust_rms=7.515 arcsec worst_quadrant_rms=43.249 arcsec
SIP_REFIT: SIP order 3 trial: matched=4727 robust_rms=0.547 arcsec worst_quadrant_rms=0.634 arcsec
SIP_REFIT: SIP order 5 trial: matched=4727 robust_rms=0.451 arcsec worst_quadrant_rms=0.573 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4727 robust_rms_before=0.463 arcsec robust_rms_before_corrected=0.576 arcsec robust_rms_after=0.451 arcsec worst_quadrant_rms_before=0.623 worst_quadrant_rms_after=0.573
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.623 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits N_match=4727 sigma_overall_arcsec=0.573 sigma_q1_arcsec=0.575 sigma_q2_arcsec=0.721 sigma_q3_arcsec=0.539 sigma_q4_arcsec=0.606 n_q1=1158 n_q2=477 n_q3=2416 n_q4=676 worst_quadrant_to_overall_ratio=1.259
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits -region wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.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.IbfUWBA2Iq (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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=539, bad_region=1, passed=19500
Got 19500 stars (including 18924 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat
util/solve_plate_with_UCAC5 got 19500 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.4 to 19.5)
Done reading UCAC5 zone files...
Matched 4817 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 4732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 19482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 491 to 549 (Dec 8.4 to 19.5)
Done reading UCAC5 zone files...
Matched 4818 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4737 matched stars entering correct_measured_positions(), 19481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4737 matched stars entering correct_measured_positions(), 19481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4737 stars left (next iteration limit 5209)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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=4737 robust_rms=8.389 arcsec worst_quadrant_rms=26.064 arcsec
SIP_REFIT: SIP order 3 trial: matched=4737 robust_rms=0.514 arcsec worst_quadrant_rms=0.645 arcsec
SIP_REFIT: SIP order 5 trial: matched=4737 robust_rms=0.433 arcsec worst_quadrant_rms=0.555 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4737 robust_rms_before=0.435 arcsec robust_rms_before_corrected=0.523 arcsec robust_rms_after=0.433 arcsec worst_quadrant_rms_before=0.559 worst_quadrant_rms_after=0.555
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.559 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits N_match=4737 sigma_overall_arcsec=0.534 sigma_q1_arcsec=0.546 sigma_q2_arcsec=0.698 sigma_q3_arcsec=0.468 sigma_q4_arcsec=0.555 n_q1=1391 n_q2=572 n_q3=2121 n_q4=653 worst_quadrant_to_overall_ratio=1.307
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Ori-02-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits -region wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-36-53_20.00sec_-0.00C_LIGHTs_0095.fits
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.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-Q1b1x1_063832_TTUQ1b1x1_3774353_9QFQ4Atl/wcs_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096.fits
Preparing the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:44:33.03 +14:56:53.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:30.89 +13:22:15.7: 11.84 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:14.71 +13:23:20.8: 12.15 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:47.76 +14:35:55.4: 12.74 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:36.57 +13:54:59.3: 12.26 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:33.48 +13:31:10.2: 12.73 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:44:33.03 +14:56:53.2: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:47.25 +14:10:05.8: 13.09 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:57:29.11 +15:42:53.0: 13.06 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:42:55.06 +13:34:38.6: 12.93 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:30.89 +13:22:15.7: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry filter KEPT candidate at 06:34:30.89 +13:22:15.7: ref_mag=11.83 +/- 0.01 new_mean_mag=10.9226 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:14.71 +13:23:20.8: 12.15 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:36.57 +13:54:59.3: 12.27 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:47.76 +14:35:55.4: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:33.48 +13:31:10.2: 12.72 +/- 0.02 detection
Forced photometry filter KEPT candidate at 06:34:14.71 +13:23:20.8: ref_mag=12.15 +/- 0.01 new_mean_mag=11.1934 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 06:34:36.57 +13:54:59.3: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2797 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 05:43:47.76 +14:35:55.4: ref_mag=12.79 +/- 0.01 new_mean_mag=11.8638 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 06:34:33.48 +13:31:10.2: ref_mag=12.72 +/- 0.01 new_mean_mag=11.6214 delta=1.10 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:57:29.11 +15:42:53.0: 13.03 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:47.25 +14:10:05.8: 13.20 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:42:55.06 +13:34:38.6: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 05:57:29.11 +15:42:53.0: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0516 delta=0.99 (need > 0.90)
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 05:43:47.25 +14:10:05.8: ref_mag=13.14 +/- 0.02 new_mean_mag=12.0356 delta=1.10 (need > 0.90)
Forced photometry filter KEPT candidate at 05:42:55.06 +13:34:38.6: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9913 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:37.50 +14:16:13.0: 13.11 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:37.50 +14:16:13.0: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 05:43:37.50 +14:16:13.0: ref_mag=13.12 +/- 0.02 new_mean_mag=12.0793 delta=1.05 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:00:54.72 +14:40:24.2: 13.11 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:49:37.58 +17:24:20.6: 13.08 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:49:11.49 +17:39:47.2: 13.06 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:00:54.72 +14:40:24.2: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 06:00:54.72 +14:40:24.2: ref_mag=13.11 +/- 0.02 new_mean_mag=11.9427 delta=1.16 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:49:37.58 +17:24:20.6: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 05:49:37.58 +17:24:20.6: ref_mag=13.08 +/- 0.02 new_mean_mag=12.1288 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:49:11.49 +17:39:47.2: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 05:49:11.49 +17:39:47.2: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1009 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:00:03.13 +14:47:30.9: 13.05 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:00:03.13 +14:47:30.9: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 06:00:03.13 +14:47:30.9: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0376 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:37.50 +14:23:14.3: 13.05 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:37.50 +14:23:14.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 05:43:37.50 +14:23:14.3: ref_mag=13.10 +/- 0.02 new_mean_mag=12.0081 delta=1.09 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:34.93 +14:23:46.5: 13.01 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:34.93 +14:23:46.5: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 05:43:34.93 +14:23:46.5: ref_mag=13.06 +/- 0.02 new_mean_mag=12.0621 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:50:10.50 +17:38:30.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:43:13.18 +14:04:44.0: 12.83 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:50:10.50 +17:38:30.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 05:50:10.50 +17:38:30.8: ref_mag=12.97 +/- 0.02 new_mean_mag=12.0258 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:48:36.66 +17:38:47.6: 12.51 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:43:13.18 +14:04:44.0: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry filter KEPT candidate at 05:43:13.18 +14:04:44.0: ref_mag=12.86 +/- 0.02 new_mean_mag=11.8559 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:42:48.30 +13:50:55.6: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:48:36.66 +17:38:47.6: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter REJECTED candidate at 05:48:36.66 +17:38:47.6: ref_mag=12.51 +/- 0.01 new_mean_mag=11.7359 delta=0.78 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:42:48.30 +13:50:55.6: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 05:42:48.30 +13:50:55.6: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8516 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:44:14.46 +14:39:59.5: 12.58 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:44:14.46 +14:39:59.5: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 05:44:14.46 +14:39:59.5: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6877 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:33.18 +13:29:53.2: 12.38 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:33:53.80 +13:29:54.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:33.18 +13:29:53.2: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter KEPT candidate at 06:34:33.18 +13:29:53.2: ref_mag=12.37 +/- 0.01 new_mean_mag=11.3000 delta=1.07 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:33:53.80 +13:29:54.3: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter KEPT candidate at 06:33:53.80 +13:29:54.3: ref_mag=12.29 +/- 0.01 new_mean_mag=11.2386 delta=1.05 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:33:48.25 +13:26:59.1: 12.27 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:50.70 +13:26:13.7: 12.22 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:33:48.25 +13:26:59.1: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter KEPT candidate at 06:33:48.25 +13:26:59.1: ref_mag=12.28 +/- 0.01 new_mean_mag=11.3633 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:50.70 +13:26:13.7: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry filter REJECTED candidate at 06:34:50.70 +13:26:13.7: ref_mag=12.21 +/- 0.01 new_mean_mag=11.3189 delta=0.90 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:00.94 +13:36:34.1: 11.78 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:00.94 +13:36:34.1: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter KEPT candidate at 06:34:00.94 +13:36:34.1: ref_mag=11.77 +/- 0.01 new_mean_mag=10.8117 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:03.23 +13:38:21.2: 11.62 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:03.23 +13:38:21.2: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.00
Forced photometry filter REJECTED candidate at 06:34:03.23 +13:38:21.2: ref_mag=11.62 +/- 0.00 new_mean_mag=10.7218 delta=0.90 (need > 0.90)
Adding exclusion_list_local.txt__out104837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99963.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 30s
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: 13s
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Considering the candidate 266155_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 266155_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
**** FOUND 06:08:32.04 +13:58:00.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 266351_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 266351_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
**** FOUND 05:49:44.46 +17:01:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266451_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 266451_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
**** FOUND 05:50:23.62 +14:19:33.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266615_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 266615_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 217685_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 217685_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
**** FOUND 06:02:23.19 +09:38:50.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129249_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 129249_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 128792_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 128792_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 116444_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 116444_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 125645_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 125645_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 99827_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 99827_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 123862_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 123862_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 110103_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 110103_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 74878_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 74878_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 107618_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 107618_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 99963_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 99963_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 36846_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 36846_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 31627_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 31627_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 97144_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 97144_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 104840_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 104840_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 104837_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 104837_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 32148_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 32148_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 112020_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 112020_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 31845_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 31845_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
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Considering the candidate 117472_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 117472_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 98231_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 98231_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 147876_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 147876_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
**** FOUND 05:56:03.29 +12:39:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126488_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 126488_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 126413_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 126413_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 127604_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 127604_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 127805_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 127805_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
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Considering the candidate 123810_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
Preparing report for the candidate 123810_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
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Considering the candidate 123261_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 123261_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
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Considering the candidate 114333_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 114333_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
**** FOUND 06:11:56.46 +14:12:27.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 114108_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 114108_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
**** FOUND 06:33:36.01 +14:09:14.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 135850_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 135850_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
**** FOUND 06:43:59.17 +13:13:36.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 62388_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096
The candidate 62388_fd_Ori-02-Q1b1x1_2026-09-10_06-37-49_20.00sec_0.00C_LIGHTs_0096 did not pass the final checks
**** FOUND 06:37:42.72 +16:23:53.6 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 44s
Prepared the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:43:34.93 +14:23:46.5
05:43:37.50 +14:23:14.3
05:43:37.50 +14:16:13.0
05:43:47.25 +14:10:05.8
05:43:13.18 +14:04:44.0
06:34:36.57 +13:54:59.3
05:42:48.30 +13:50:55.6
06:34:00.94 +13:36:34.1
05:42:55.06 +13:34:38.6
06:34:33.48 +13:31:10.2
06:33:53.80 +13:29:54.3
06:34:33.18 +13:29:53.2
06:33:48.25 +13:26:59.1
06:34:14.71 +13:23:20.8
06:34:30.89 +13:22:15.7
05:44:33.03 +14:56:53.2
05:49:11.49 +17:39:47.2
05:50:10.50 +17:38:30.8
05:49:37.58 +17:24:20.6
05:57:29.11 +15:42:53.0
06:00:03.13 +14:47:30.9
05:44:14.46 +14:39:59.5
05:43:47.76 +14:35:55.4
06:00:54.72 +14:40:24.2
########### Completed Ori-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:44:33.03 +14:56:53.2
06:34:30.89 +13:22:15.7
06:34:14.71 +13:23:20.8
06:34:36.57 +13:54:59.3
06:34:33.48 +13:31:10.2
05:43:47.76 +14:35:55.4
05:42:55.06 +13:34:38.6
05:43:47.25 +14:10:05.8
05:57:29.11 +15:42:53.0
05:43:37.50 +14:16:13.0
06:00:54.72 +14:40:24.2
05:49:37.58 +17:24:20.6
05:49:11.49 +17:39:47.2
06:00:03.13 +14:47:30.9
05:43:37.50 +14:23:14.3
05:43:34.93 +14:23:46.5
05:50:10.50 +17:38:30.8
05:43:13.18 +14:04:44.0
05:42:48.30 +13:50:55.6
05:44:14.46 +14:39:59.5
06:34:33.18 +13:29:53.2
06:33:53.80 +13:29:54.3
06:33:48.25 +13:26:59.1
06:34:00.94 +13:36:34.1
###################################################################################
05:44:33.03 +14:56:53.2 -- asteroid (will NOT add it to exclusion list)
06:34:30.89 +13:22:15.7 -- not an asteroid (will add it to exclusion list)
06:34:14.71 +13:23:20.8 -- not an asteroid (will add it to exclusion list)
06:34:36.57 +13:54:59.3 -- not an asteroid (will add it to exclusion list)
06:34:33.48 +13:31:10.2 -- not an asteroid (will add it to exclusion list)
05:43:47.76 +14:35:55.4 -- not an asteroid (will add it to exclusion list)
05:42:55.06 +13:34:38.6 -- not an asteroid (will add it to exclusion list)
05:43:47.25 +14:10:05.8 -- not an asteroid (will add it to exclusion list)
05:57:29.11 +15:42:53.0 -- not an asteroid (will add it to exclusion list)
05:43:37.50 +14:16:13.0 -- not an asteroid (will add it to exclusion list)
06:00:54.72 +14:40:24.2 -- not an asteroid (will add it to exclusion list)
05:49:37.58 +17:24:20.6 -- not an asteroid (will add it to exclusion list)
05:49:11.49 +17:39:47.2 -- not an asteroid (will add it to exclusion list)
06:00:03.13 +14:47:30.9 -- not an asteroid (will add it to exclusion list)
05:43:37.50 +14:23:14.3 -- not an asteroid (will add it to exclusion list)
05:43:34.93 +14:23:46.5 -- not an asteroid (will add it to exclusion list)
05:50:10.50 +17:38:30.8 -- not an asteroid (will add it to exclusion list)
05:43:13.18 +14:04:44.0 -- not an asteroid (will add it to exclusion list)
05:42:48.30 +13:50:55.6 -- not an asteroid (will add it to exclusion list)
05:44:14.46 +14:39:59.5 -- not an asteroid (will add it to exclusion list)
06:34:33.18 +13:29:53.2 -- not an asteroid (will add it to exclusion list)
06:33:53.80 +13:29:54.3 -- not an asteroid (will add it to exclusion list)
06:33:48.25 +13:26:59.1 -- not an asteroid (will add it to exclusion list)
06:34:00.94 +13:36:34.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:42:48.30 +13:50:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:55.06 +13:34:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:13.18 +14:04:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:34.93 +14:23:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:37.50 +14:16:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:37.50 +14:23:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:47.25 +14:10:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:47.76 +14:35:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:14.46 +14:39:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:11.49 +17:39:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:37.58 +17:24:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.50 +17:38:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:29.11 +15:42:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:03.13 +14:47:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:54.72 +14:40:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:48.25 +13:26:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:53.80 +13:29:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:00.94 +13:36:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:14.71 +13:23:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:30.89 +13:22:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:33.18 +13:29:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:33.48 +13:31:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:36.57 +13:54:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:42:48.30 +13:50:55.6 -- not a known variable star
05:42:55.06 +13:34:38.6 -- not a known variable star
05:43:13.18 +14:04:44.0 -- not a known variable star
05:43:34.93 +14:23:46.5 -- a known variable star
05:43:37.50 +14:16:13.0 -- not a known variable star
05:43:37.50 +14:23:14.3 -- not a known variable star
05:43:47.25 +14:10:05.8 -- not a known variable star
05:43:47.76 +14:35:55.4 -- not a known variable star
05:44:14.46 +14:39:59.5 -- not a known variable star
05:49:11.49 +17:39:47.2 -- not a known variable star
05:49:37.58 +17:24:20.6 -- not a known variable star
05:50:10.50 +17:38:30.8 -- not a known variable star
05:57:29.11 +15:42:53.0 -- a known variable star
06:00:03.13 +14:47:30.9 -- not a known variable star
06:00:54.72 +14:40:24.2 -- a known variable star
06:33:48.25 +13:26:59.1 -- not a known variable star
06:33:53.80 +13:29:54.3 -- not a known variable star
06:34:00.94 +13:36:34.1 -- not a known variable star
06:34:14.71 +13:23:20.8 -- a known variable star
06:34:30.89 +13:22:15.7 -- not a known variable star
06:34:33.18 +13:29:53.2 -- not a known variable star
06:34:33.48 +13:31:10.2 -- not a known variable star
06:34:36.57 +13:54:59.3 -- not a known variable star
Found 19 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
23 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
05:42:48.30 +13:50:55.6
05:42:55.06 +13:34:38.6
05:43:13.18 +14:04:44.0
05:43:34.93 +14:23:46.5
05:43:37.50 +14:16:13.0
05:43:37.50 +14:23:14.3
05:43:47.25 +14:10:05.8
05:43:47.76 +14:35:55.4
05:44:14.46 +14:39:59.5
05:49:11.49 +17:39:47.2
05:49:37.58 +17:24:20.6
05:50:10.50 +17:38:30.8
05:57:29.11 +15:42:53.0
06:00:03.13 +14:47:30.9
06:00:54.72 +14:40:24.2
06:33:48.25 +13:26:59.1
06:33:53.80 +13:29:54.3
06:34:00.94 +13:36:34.1
06:34:14.71 +13:23:20.8
06:34:30.89 +13:22:15.7
06:34:33.18 +13:29:53.2
06:34:33.48 +13:31:10.2
06:34:36.57 +13:54:59.3
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461293.98406977 -observatory V36
11:58:36.50 +00:58:34.0 Mercury (-0.7mag)
13:43:49.76 -15:41:28.9 Venus (-4.7mag)
07:22:33.30 +22:46:00.2 Mars (1.2mag)
09:11:39.51 +16:46:28.7 Jupiter (-1.8mag)
00:50:58.74 +02:33:19.4 Saturn (0.4mag)
04:13:42.59 +21:02:03.2 Uranus (5.7mag)
00:13:26.51 -00:05:16.7 Neptune (7.7mag)
20:25:22.80 -23:40:19.0 Pluto (14.5mag)
10:44:08.23 +06:52:06.2 Moon (99.9mag)
-rw-r--r-- 1 apache apache 362 Sep 10 06:39 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461293.98406977:
09:11:46.90 +16:45:52.5 Io (6.2mag)
09:11:41.43 +16:46:20.3 Europa (6.3mag)
09:11:28.34 +16:47:26.9 Ganymede (5.7mag)
09:11:40.61 +16:46:25.3 Callisto (6.9mag)
09:09:32.59 +17:04:22.0 Himalia (15.7mag)
09:11:39.90 +16:46:27.1 Thebe (16.6mag)
09:09:07.66 +16:58:15.3 Elara (17.7mag)
09:15:28.34 +16:13:08.0 Pasiphae (17.9mag)
09:12:30.68 +17:05:08.1 Carme (19.0mag)
00:50:44.63 +02:33:23.7 Titan (8.3mag)
00:50:57.31 +02:33:24.2 Rhea (9.6mag)
00:51:05.11 +02:35:30.2 Iapetus (11.0mag)
00:51:13.38 +02:33:13.9 Hyperion (14.3mag)
00:49:42.23 +02:22:46.2 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 10 06:39 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461293.98406977:
22:29:26.17 +04:15:08.7 JWST
18:37:52.59 +16:31:55.4 Chandra
07:05:33.15 -06:01:14.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 10 06:39 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461293.98406977 -observatory V36
03:42:12.46 +19:28:57.1 17.3mag P/1996 R2 (Lagerkvist)
18:04:07.17 -34:09:04.9 14.4mag P/2010 H2 (Vales)
07:21:50.84 -70:28:48.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:01.77 +33:47:01.1 17.7mag C/2017 K2 (PANSTARRS)
22:10:58.18 +28:16:31.6 17.5mag C/2022 E2 (ATLAS)
07:12:33.95 +25:55:13.3 16.9mag C/2022 N2 (PANSTARRS)
10:52:25.94 +27:06:49.2 17.1mag C/2022 QE78 (ATLAS)
09:50:41.12 +05:12:55.3 18.0mag C/2022 R6 (PANSTARRS)
15:28:44.88 -15:55:42.8 14.9mag C/2023 R1 (PANSTARRS)
08:41:08.67 +33:05:34.6 15.8mag C/2024 E1 (Wierzchos)
15:07:01.96 +15:17:11.3 17.9mag C/2024 G6 (ATLAS)
18:31:43.09 +43:02:49.8 13.7mag C/2024 J3 (ATLAS)
20:21:52.56 +49:07:06.4 17.4mag C/2024 R4 (PANSTARRS)
05:37:15.21 -13:04:18.8 15.1mag C/2024 T5 (ATLAS)
07:12:40.36 +17:54:05.6 17.8mag C/2025 J1 (Borisov)
11:23:08.72 +18:31:09.6 16.8mag C/2025 V2 (Rankin)
13:22:16.59 -00:08:30.9 16.8mag C/2025 Y1 (ATLAS)
16:50:02.15 +73:29:39.6 16.0mag C/2026 A2 (Bok)
03:04:06.27 +46:01:29.0 17.5mag C/2026 B2 (Sun-Gao)
12:16:14.11 +11:32:37.2 17.5mag A/2026 E1
22:28:38.65 -35:11:58.6 13.5mag 10P/Tempel
01:24:27.41 +37:39:35.6 17.8mag 11P/Tempel-Swift-LINEAR
11:50:18.65 -05:42:31.9 16.3mag 29P/Schwassmann-Wachmann
12:14:59.45 -06:06:00.8 17.7mag 63P/Wild
06:45:26.31 +19:00:11.8 13.7mag 78P/Gehrels
03:17:18.41 +15:01:47.8 17.2mag 88P/Howell
05:48:53.04 +29:50:36.2 16.9mag 112P/Urata-Niijima
07:41:11.62 +23:59:03.6 15.9mag 114P/Wiseman-Skiff
10:34:59.53 +20:11:17.3 14.8mag 123P/West-Hartley
12:53:39.18 -22:26:34.8 17.5mag 124P/Mrkos
06:21:13.62 +20:32:17.4 15.9mag 128P/Shoemaker-Holt
02:18:43.47 -17:10:33.8 14.9mag 161P/Hartley-IRAS
09:01:49.28 +37:28:12.2 16.4mag 162P/Siding Spring
09:33:18.81 +11:51:38.6 13.2mag 169P/NEAT
03:26:56.17 +08:12:06.6 14.5mag 220P/McNaught
04:56:35.24 +37:18:18.3 15.2mag 260P/McNaught
08:40:22.09 +35:21:21.4 17.3mag 295P/LINEAR
15:27:20.46 -00:36:22.5 17.9mag 391P/Kowalski
09:30:31.58 +16:41:16.1 17.8mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.0K Sep 10 06:39 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
-rw-r--r-- 1 apache apache 5.7K Sep 10 06:39 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 10 06:39 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
01:10:34.560 -00:57:04.24 AT 2026yyl 2026-08-06.84 21.95
23:32:11.290 +02:22:43.17 AT 2026yyk 2026-08-06.82 22.15
00:08:51.810 +05:23:51.48 AT 2026yyj 2026-08-06.76 22.29
22:56:29.190 +05:38:34.33 AT 2026yyi 2026-08-06.74 22.59
00:15:40.360 +03:16:53.74 AT 2026yyh 2026-08-04.79 21.17
23:43:25.860 +04:21:29.59 AT 2026yyg 2026-08-04.79 20.76
01:06:50.820 +00:11:19.23 AT 2026yyf 2026-08-01.81 21.09
13:53:44.240 -01:14:56.96 AT 2026yye 2026-07-21.61 20.99
23:54:21.350 +02:49:56.21 AT 2026yyd 2026-07-15.87 22.7
23:59:00.130 +05:02:18.24 AT 2026yyc 2026-08-09.84 21.93
02:17:16.710 -00:36:33.05 AT 2026yyb 2026-07-30.82 20.03
02:27:18.740 +05:57:45.58 AT 2026yya 2026-08-01.84 20.95
01:29:14.660 +04:56:12.14 AT 2026yxz 2026-08-06.84 21.5
05:02:13.153 +13:11:04.42 AT 2026yxy 2026-07-19.50 18.8535
22:01:35.905 -00:50:35.09 AT 2026yxx 2026-08-12.32 19.906
16:14:10.014 -14:08:40.56 AT 2026yxw 2026-08-12.88 19.268
02:19:09.961 +30:43:26.21 AT 2026yxv 2026-08-14.56 19.34
13:13:44.418 +06:59:28.07 AT 2026yxu 2026-08-05.16 19.7272
14:52:44.979 +53:35:27.83 AT 2026yxt 2026-08-05.18 20.8609
00:56:58.931 +27:08:48.44 SN 2026yxs 2026-08-15.06 19.27
-rw-r--r-- 1 apache apache 88K Sep 10 06:39 tns_transients_list.txt
