This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds
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 10 09.3670 2461322.8670 12.65 02:49:53.57 +17:46:31.0
158.86782 -36.69769 galactic Ari Second-epoch detections are separated by 0.5" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.419 Aurelia -0 0 0 12.8 -0 -0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:49:53.57 +17:46:31.0: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:49:53.57 +17:46:31.0: 16.10 +/- 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 10 09.3670* 02 49 53.57 +17 46 31.0 12.7 U Ari 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,2461322.8670,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.3670 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.3670 2461322.8670 13.06 03:02:32.45 +15:47:58.3
163.37035 -36.57511 galactic Ari Second-epoch detections are separated by 0.6" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.149 Medusa -0 -0 0 13.2 0 0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:02:32.45 +15:47:58.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:02:32.45 +15:47:58.3: 16.07 +/- 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 10 09.3670* 03 02 32.45 +15 47 58.3 13.1 U Ari 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,2461322.8670,13.06,0.05,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
VARIABLE_NAME 20261009.3670 13.06CV 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 10 09.3670 2461322.8670 13.51 02:25:28.72 +14:05:13.3
154.80833 -42.88916 galactic Ari Second-epoch detections are separated by 0.7" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.257 Silesia -0 0 0 13.9 -0 -0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:25:28.72 +14:05:13.3: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:25:28.72 +14:05:13.3: 16.20 +/- 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 10 09.3670* 02 25 28.72 +14 05 13.3 13.5 U Ari 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,2461322.8670,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.3670 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.3670 2461322.8670 13.91 02:47:08.56 +15:37:24.0
159.67143 -38.85667 galactic Ari Second-epoch detections are separated by 2.1" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.494 Virtus 1 -0 1 14.1 -0 -0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:47:08.56 +15:37:24.0: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:47:08.56 +15:37:24.0: 16.24 +/- 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 10 09.3670* 02 47 08.56 +15 37 24.0 13.9 U Ari 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,2461322.8670,13.91,0.05,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
VARIABLE_NAME 20261009.3670 13.91CV 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 10 09.3670 2461322.8670 14.12 02:34:12.06 +18:54:28.9
154.13397 -37.65981 galactic Ari Second-epoch detections are separated by 1.2" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.248 Lameia 0 0 0 14.1 -0 0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:34:12.06 +18:54:28.9: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:34:12.06 +18:54:28.9: 16.14 +/- 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 10 09.3670* 02 34 12.06 +18 54 28.9 14.1 U Ari 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,2461322.8670,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.3670 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.3670 2461322.8670 14.20 02:25:08.91 +10:20:58.5
157.31990 -46.17138 galactic Cet Second-epoch detections are separated by 2.6" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.99 Dike -1 -1 1 14.1 0 -0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:25:08.91 +10:20:58.5: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:25:08.91 +10:20:58.5: 16.06 +/- 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 10 09.3670* 02 25 08.91 +10 20 58.5 14.2 U Cet 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,2461322.8670,14.20,0.05,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 20261009.3670 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.3670 2461322.8670 14.78 02:47:25.88 +13:10:19.3
161.53991 -40.84585 galactic Ari Second-epoch detections are separated by 1.3" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1621 Druzhba -0 -0 0 14.2 0 0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:47:25.88 +13:10:19.3: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:47:25.88 +13:10:19.3: 16.22 +/- 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 10 09.3670* 02 47 25.88 +13 10 19.3 14.8 U Ari 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,2461322.8670,14.78,0.05,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 20261009.3670 14.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.3670 2461322.8670 14.86 02:56:06.47 +15:12:43.4
162.23815 -37.96617 galactic Ari Second-epoch detections are separated by 0.7" 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.936 Kunigunde -0 1 1 15.1 -0 0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:56:06.47 +15:12:43.4: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:56:06.47 +15:12:43.4: 16.12 +/- 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 10 09.3670* 02 56 06.47 +15 12 43.4 14.9 U Ari 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,2461322.8670,14.86,0.05,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
VARIABLE_NAME 20261009.3670 14.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.3670 2461322.8670 15.04 03:06:36.22 +08:48:45.9
170.02599 -41.37992 galactic Cet Second-epoch detections are separated by 3.3" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.4272 Entsuji 1 -1 2 14.8 -0 -0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:06:36.22 +08:48:45.9: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:06:36.22 +08:48:45.9: 15.80 +/- 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 10 09.3670* 03 06 36.22 +08 48 45.9 15.0 U Cet 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,2461322.8670,15.04,0.05,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
VARIABLE_NAME 20261009.3670 15.04CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.65708573 09.01.2026 03:46:02.207 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
First image: 2461049.65708573 09.01.2026 03:46:02.207 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Last image: 2461322.86729515 09.10.2026 08:48:44.301 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7673
Objects passed selection criteria: 7671
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7274.5
Average stars matched: 7051.5 (96.9345 %)
Memory usage VmPeak: 233548 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 03:53:30 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: 2461049.65708573 09.01.2026 03:46:02.207 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
First image: 2461049.65708573 09.01.2026 03:46:02.207 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Last image: 2461322.86729515 09.10.2026 08:48:44.301 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 101
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.07
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: 17 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): 44709
Objects passed selection criteria: 44592
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 42909.8
Average stars matched: 40592 (94.5985 %)
Memory usage VmPeak: 267548 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 03:54:28 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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
SExtractor catalog cache: saved Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.cat to cache
SExtractor catalog cache: saved Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461322.86664446
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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits exists and is non-empty
wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits exists and is non-empty
wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits exists and is non-empty
wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits (1st reference image)
verification OK: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Image size: 941.6'x627.0' 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: 02:40:00.532 +13:59:54.76 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_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits (1st new image)
verification OK: wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
Image size: 941.4'x626.8' 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: 02:40:01.058 +13:59:50.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:40:00.532 +13:59:54.76
Second-epoch image center 02:40:01.058 +13:59:50.02
Angular distance between the image centers 0.0025 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits (2nd new image)
verification OK: wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
Image size: 941.4'x626.8' 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: 02:39:58.600 +13:59:08.87 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:40:00.532 +13:59:54.76
Second-epoch image center 02:39:58.600 +13:59:08.87
Angular distance between the image centers 0.0149 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 02:40:01.058 +13:59:50.02
Second-epoch second image center 02:39:58.600 +13:59:08.87
Angular distance between the image centers 0.01515 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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits &> /tmp/tmp.gs5nvxOlWU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits &> /tmp/tmp.KXYB5yokpY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits &> /tmp/tmp.Z8tZwjyiLP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits &> /tmp/tmp.ScFOV7zM31
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits and wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits and wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat
Found non-empty wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits and wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat
The reference image (wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits) and catalog (wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat) found
'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat' -> 'wcsmag.cat'
Read 7398 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.7516 to 48.3015 deg, Dec +8.6571 to +19.2857 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 31.7516 to 48.3015 deg, Dec 8.6571 to 19.2857 deg
Loaded 4349 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): 3551 out of 3736 total matches.
Matched with Tycho-2 3736 out of 7398 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.949700
a=0.000000 b=1.000000 c=22.949700
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7398 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.7516 to 48.3015 deg, Dec +8.6571 to +19.2857 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 31.7516 to 48.3015 deg, Dec 8.6571 to 19.2857 deg
Loaded 4349 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): 3551 out of 3736 total matches.
Matched with Tycho-2 3736 out of 7398 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Forced-photometry filter: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits -> calib.txt_param_ref_wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits (aperture=6.1)
Read 7374 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.7516 to 48.3014 deg, Dec +8.6570 to +19.2905 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 31.7516 to 48.3014 deg, Dec 8.6570 to 19.2905 deg
Loaded 4352 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): 3558 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7374 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Forced-photometry filter: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits -> calib.txt_param_ref_wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
2.0 pix Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
2.1 pix fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
2.1 pix fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
Limiting magnitude estimates:
15.6 mag. Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
15.6 mag. Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
15.6 mag. fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
15.6 mag. fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
All-image limiting magnitude estimate: 15.6 (SNR ) 12.3 (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.gs5nvxOlWU (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_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits' -> 'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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=508, bad_region=0, passed=7398
Got 7398 stars (including 6885 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat
util/solve_plate_with_UCAC5 got 7398 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 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 4882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 7398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
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 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 7398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 7398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4882 stars left (next iteration limit 5370)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits N_match=4882 sigma_overall_arcsec=0.258 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.253 sigma_q3_arcsec=0.237 sigma_q4_arcsec=0.213 n_q1=1360 n_q2=1218 n_q3=1081 n_q4=1223 worst_quadrant_to_overall_ratio=1.288
The image catalog is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits -region wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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.KXYB5yokpY (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_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits' -> 'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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=503, bad_region=0, passed=7374
Got 7374 stars (including 6862 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat
util/solve_plate_with_UCAC5 got 7374 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 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
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 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4887 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits N_match=4887 sigma_overall_arcsec=0.272 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.261 sigma_q3_arcsec=0.250 sigma_q4_arcsec=0.233 n_q1=1370 n_q2=1212 n_q3=1075 n_q4=1230 worst_quadrant_to_overall_ratio=1.256
The image catalog is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits -region wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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.Z8tZwjyiLP (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_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.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_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.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=505, bad_region=0, passed=7254
Got 7254 stars (including 6735 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
util/solve_plate_with_UCAC5 got 7254 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 4882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 7254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 7254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 7254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4882 stars left (next iteration limit 5370)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4882 robust_rms=13.098 arcsec worst_region_rms=28.617 arcsec outer_annulus_rms=28.617 arcsec
SIP_REFIT: SIP order 3 trial: matched=4882 robust_rms=0.569 arcsec worst_region_rms=0.647 arcsec outer_annulus_rms=0.647 arcsec
SIP_REFIT: SIP order 5 trial: matched=4882 robust_rms=0.349 arcsec worst_region_rms=0.416 arcsec outer_annulus_rms=0.303 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4882 robust_rms_before=1.096 arcsec robust_rms_before_corrected=0.345 arcsec robust_rms_after=0.349 arcsec worst_region_rms_before=0.408 worst_region_rms_after=0.416 outer_annulus_rms_before=1.227 outer_annulus_rms_after=0.303
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.408 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits worst_region_rms_kept=0.408 arcsec robust_rms_kept=0.345 arcsec matched=4882
WCS_QUALITY_DIAG: file=fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits N_match=4882 sigma_overall_arcsec=0.354 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.409 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.325 n_q1=1389 n_q2=1195 n_q3=1086 n_q4=1212 worst_quadrant_to_overall_ratio=1.153
The image catalog is written to wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits -region wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.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.ScFOV7zM31 (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_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.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_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.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=511, bad_region=0, passed=7229
Got 7229 stars (including 6710 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat
util/solve_plate_with_UCAC5 got 7229 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 4879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 7229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 7229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 7229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4879 stars left (next iteration limit 5366)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4879 robust_rms=13.041 arcsec worst_region_rms=28.681 arcsec outer_annulus_rms=28.681 arcsec
SIP_REFIT: SIP order 3 trial: matched=4879 robust_rms=0.584 arcsec worst_region_rms=0.689 arcsec outer_annulus_rms=0.689 arcsec
SIP_REFIT: SIP order 5 trial: matched=4879 robust_rms=0.347 arcsec worst_region_rms=0.427 arcsec outer_annulus_rms=0.299 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4879 robust_rms_before=1.122 arcsec robust_rms_before_corrected=0.352 arcsec robust_rms_after=0.347 arcsec worst_region_rms_before=0.438 worst_region_rms_after=0.427 outer_annulus_rms_before=1.213 outer_annulus_rms_after=0.299
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.438 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits worst_region_rms_kept=0.438 arcsec robust_rms_kept=0.352 arcsec matched=4879
WCS_QUALITY_DIAG: file=fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits N_match=4879 sigma_overall_arcsec=0.354 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.420 sigma_q3_arcsec=0.341 sigma_q4_arcsec=0.324 n_q1=1385 n_q2=1178 n_q3=1095 n_q4=1221 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits -region wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits to local_wcs_cache/
'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits' -> 'local_wcs_cache/wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits'
Saving the final (post-refit) wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits to local_wcs_cache/
'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits' -> 'local_wcs_cache/wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits'
Saving the final (post-refit) wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits to local_wcs_cache/
'wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits'
Saving the final (post-refit) wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits to local_wcs_cache/
'wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits sigma_overall=0.258 worst_q_ratio=1.288
ref2=Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits sigma_overall=0.272 worst_q_ratio=1.256
new1=fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits sigma_overall=0.354 worst_q_ratio=1.153
new2=fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits sigma_overall=0.354 worst_q_ratio=1.185
reference average sigma_overall=0.265 worst_q_ratio=1.272
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117_astrometric_residuals.png (4882 matched stars from wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118_astrometric_residuals.png (4887 matched stars from wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428_astrometric_residuals.png (4882 matched stars from wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429_astrometric_residuals.png (4879 matched stars from wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-47-48_20.00sec_-0.00C_LIGHTs_0428.fits'
Saving fully-calibrated image wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Ari-04-Q1b1x1_035115_TTUQ1b1x1_217538_A0jTF1Ds/wcs_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429.fits'
Preparing the HTML report for the field Ari-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:03:56.21 +13:11:12.4: 12.29 +/- 0.01 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:03:56.21 +13:11:12.4: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter REJECTED candidate at 03:03:56.21 +13:11:12.4: ref_mag=12.30 +/- 0.01 new_mean_mag=12.3653 delta=-0.06 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
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Considering the candidate 20359_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 20359_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 05052_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 05052_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53127_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53127_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53128_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53128_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53133_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53133_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53135_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53135_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53137_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53137_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53140_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53140_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53142_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53142_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53143_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53143_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53146_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53146_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53147_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53147_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53149_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53149_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53150_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53150_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53153_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53153_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53156_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53156_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53162_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53162_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53164_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53164_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53167_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53167_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53168_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53168_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53173_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53173_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53175_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53175_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53176_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53176_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53177_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53177_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53182_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53182_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53183_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53183_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53189_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53189_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53202_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53202_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53355_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
Preparing report for the candidate 53355_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
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Considering the candidate 53389_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53389_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53437_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
Preparing report for the candidate 53437_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
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Considering the candidate 53581_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
Preparing report for the candidate 53581_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
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Considering the candidate 53804_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
Preparing report for the candidate 53804_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
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Considering the candidate 53889_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
Preparing report for the candidate 53889_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
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Considering the candidate 53969_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 53969_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54002_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
Preparing report for the candidate 54002_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
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Considering the candidate 54058_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54058_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54108_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54108_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54113_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54113_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 54342_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54342_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54348_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
Preparing report for the candidate 54348_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
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Considering the candidate 54355_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54355_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54369_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54369_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
**** FOUND 03:07:28.07 +17:51:11.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54377_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54377_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54379_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54379_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54383_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54383_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54390_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54390_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54436_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54436_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54445_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
Preparing report for the candidate 54445_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
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Considering the candidate 54451_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54451_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54456_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54456_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54475_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54475_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54480_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54480_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54490_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54490_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54493_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54493_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54497_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54497_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54510_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54510_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54518_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54518_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54519_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54519_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54536_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54536_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54546_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54546_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54558_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54558_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54564_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54564_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54566_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54566_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54567_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54567_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54578_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54578_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54579_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54579_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54580_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54580_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54594_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54594_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54597_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54597_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54599_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54599_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54601_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54601_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54614_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
Preparing report for the candidate 54614_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
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Considering the candidate 54618_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54618_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54620_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54620_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54625_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54625_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54630_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54630_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54633_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54633_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54639_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54639_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54644_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54644_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54650_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54650_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54652_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54652_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54658_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54658_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54675_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54675_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54684_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54684_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54686_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54686_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54711_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54711_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54727_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54727_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54745_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54745_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54758_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54758_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54792_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 54792_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 41054_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429
The candidate 41054_fd_Ari-04-Q1b1x1_2026-10-09_03-48-44_20.00sec_-0.00C_LIGHTs_0429 did not pass the final checks
