This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3757204512567291904,2461136.7114,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3757204512567291904 20260406.2114 11.03CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3750081292126774656,2461136.7114,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3750081292126774656 20260406.2114 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 06.2114 2461136.7114 10.04 10:45:38.23 -13:37:11.4
262.14001 39.08842 galactic Hya Second-epoch detections are separated by 0.9" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3750336172666209280 | 10:45:37.91 -13:37:15.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F7V 1988MSS...C04....0H HD 93217
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3750336172666209280,2461136.7114,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3750336172666209280 20260406.2114 10.04CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RT Crt,2461136.7114,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RT Crt 20260406.2114 10.84CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7114,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2114 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7114,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2114 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7114,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2114 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3757418363283130368,2461136.7114,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3757418363283130368 20260406.2114 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 04 06.2114* 10 44 53.43 -11 19 59.2 12.5 U Sex 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3757645618592350848,2461136.7114,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3757645618592350848 20260406.2114 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J161.4828-13.0348,2461136.7114,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J161.4828-13.0348 20260406.2114 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J161.3656-13.7150,2461136.7114,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J161.3656-13.7150 20260406.2114 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J161.5369-12.1375,2461136.7114,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J161.5369-12.1375 20260406.2114 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3750310952618092032,2461136.7114,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3750310952618092032 20260406.2114 12.16CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3750246734267196160,2461136.7114,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3750246734267196160 20260406.2114 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3751210146971117696,2461136.7114,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3751210146971117696 20260406.2114 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3751113767905080704,2461136.7114,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3751113767905080704 20260406.2114 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 04 06.2114* 10 45 29.55 -08 52 35.4 11.9 U Sex 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3761589463721973120,2461136.7114,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3761589463721973120 20260406.2114 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3750252437983719680,2461136.7114,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3750252437983719680 20260406.2114 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3750267762427103488,2461136.7114,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3750267762427103488 20260406.2114 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3750245119359490432,2461136.7114,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3750245119359490432 20260406.2114 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3750318133803443584,2461136.7114,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3750318133803443584 20260406.2114 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 04 06.2114* 10 44 26.22 -08 22 22.1 11.6 U Sex 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3762394100075107584,2461136.7114,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3762394100075107584 20260406.2114 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3757148128236358784,2461136.7114,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3757148128236358784 20260406.2114 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 04 06.2114* 10 44 30.56 -08 23 32.4 10.8 U Sex 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3762393275441387392,2461136.7114,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3762393275441387392 20260406.2114 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7114,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2114 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1053280-081809,2461136.7114,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1053280-081809 20260406.2114 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461136.71163378 06.04.2026 05:04:35.159 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6328
Objects passed selection criteria: 6304
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 5204.75
Average stars matched: 4845.5 (93.0977 %)
Memory usage VmPeak: 111784 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:10:13 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461136.71163378 06.04.2026 05:04:35.159 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 270
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.44
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: 14 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 36009
Objects passed selection criteria: 35880
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 27593.2
Average stars matched: 25840.2 (93.647 %)
Memory usage VmPeak: 137312 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:11:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.71111747
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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
Saving wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits to local_wcs_cache/
'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> 'local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
Saving wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits to local_wcs_cache/
'wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> 'local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits'
wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:37.783 -09:59:16.33
Angular distance between the image centers 0.0742 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:37.298 -09:59:18.89
Angular distance between the image centers 0.0721 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 11:08:37.783 -09:59:16.33
Second-epoch second image center 11:08:37.298 -09:59:18.89
Angular distance between the image centers 0.00211 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.71917Yh19y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.CbLKr2fVMN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits &> /tmp/tmp.JPwGPnHsWa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits &> /tmp/tmp.YHoDWHIlIQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat' -> 'wcsmag.cat'
Read 6631 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.9881 to 175.1919 deg, Dec -15.3070 to -4.7038 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 158.9881 to 175.1919 deg, Dec -15.3070 to -4.7038 deg
Loaded 4601 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): 3732 out of 3905 total matches.
Matched with Tycho-2 3905 out of 6631 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.839875
a=0.000000 b=1.000000 c=22.839875
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
2.0 pix Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
4.7 pix fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
4.7 pix fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Limiting magnitude estimates:
15.1 mag. Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
15.1 mag. Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
14.3 mag. fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
14.3 mag. fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.8 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.71917Yh19y (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=466, passed=6631
Got 6631 stars (including 6155 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 6631 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.CbLKr2fVMN (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=470, passed=6561
Got 6561 stars (including 6079 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 6561 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6503 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JPwGPnHsWa (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_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.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_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=749, passed=5655
Got 5655 stars (including 4902 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 5655 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.6'
Seting catalog search parameters based on the expected field of view 936.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013008 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010407 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5405 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5402 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5402 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits -region wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.YHoDWHIlIQ (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_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.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_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Checking if the catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
WCS catalog name: wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=811, passed=5702
Got 5702 stars (including 4887 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat
util/solve_plate_with_UCAC5 got 5702 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.6'
Seting catalog search parameters based on the expected field of view 936.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013008 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010407 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits -region wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
Saving fully-calibrated image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
Saving fully-calibrated image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits'
Saving fully-calibrated image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits'
Preparing the HTML report for the field Crt-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20303.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20283_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 20283_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:45:48.23 -13:27:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 3.207 3751113767905080704 161.45184654067 -13.44980984335 11.3908 10.9426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20293_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 20293_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20294_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 20294_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20303_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 20303_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20304_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 20304_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:46:43.80 -14:04:49.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20522_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 20522_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:48:49.08 -09:00:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04837_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 04837_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 20s
Prepared the HTML report for the field Crt-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:01:55.26 -07:39:43.8
10:45:06.68 -12:45:42.2
10:48:45.03 -14:06:19.5
10:45:38.23 -13:37:11.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Creating symlink local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits exists and is non-empty
wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:37.783 -09:59:16.33
Angular distance between the image centers 0.0742 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:37.298 -09:59:18.89
Angular distance between the image centers 0.0721 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 11:08:37.783 -09:59:16.33
Second-epoch second image center 11:08:37.298 -09:59:18.89
Angular distance between the image centers 0.00211 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.63FLDa5yAM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.N31yTM9Jcn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits &> /tmp/tmp.44XzVkn9eI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits &> /tmp/tmp.FMgIeTJmG8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat' -> 'wcsmag.cat'
Read 40110 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.9737 to 175.2111 deg, Dec -15.3080 to -4.7013 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 158.9737 to 175.2111 deg, Dec -15.3080 to -4.7013 deg
Loaded 4615 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): 3663 out of 4023 total matches.
Matched with Tycho-2 4023 out of 40110 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.714876
a=0.000000 b=1.000000 c=22.714876
From vast_summary.log: estimated ref. image limiting mag.: -7.44
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.27
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.27
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 148 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
1.9 pix Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
4.1 pix fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
3.9 pix fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Limiting magnitude estimates:
15.3 mag. Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
15.3 mag. Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
14.6 mag. fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
14.6 mag. fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.63FLDa5yAM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1646, passed=40101
Got 40101 stars (including 38397 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 40101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 39628 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 39629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 39628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.N31yTM9Jcn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1596, passed=40499
Got 40499 stars (including 38842 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 40499 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 40100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 40102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 40101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.44XzVkn9eI (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_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.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_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=3401, passed=22789
Got 22789 stars (including 19384 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 22789 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.6'
Seting catalog search parameters based on the expected field of view 936.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013008 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010407 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 21780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 21782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 21782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits -region wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FMgIeTJmG8 (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_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.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_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Checking if the catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
WCS catalog name: wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=3772, passed=23602
Got 23602 stars (including 19822 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat
util/solve_plate_with_UCAC5 got 23602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.6'
Seting catalog search parameters based on the expected field of view 936.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013008 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010407 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits -region wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Saving fully-calibrated image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Saving fully-calibrated image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-03-50_20.00sec_-4.90C_LIGHT_0160.fits
Saving fully-calibrated image wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Crt-01-Q2b1x1_000511_TTUQ2b1x1_21917_GVHyBWQQ/wcs_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161.fits
Preparing the HTML report for the field Crt-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52956.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out39066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55989.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 35s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 13s
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Considering the candidate 52876_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52876_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:46:25.66 -09:02:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.029 3761571016838196352 161.60718658269 -09.04607576527 13.3058 12.8515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52882_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52882_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:45:12.57 -09:01:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.111 3761581183025032320 161.30263000062 -09.02690068475 13.2714 12.8034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52884_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52884_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:52:52.01 -12:21:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.752 3756543255106294528 163.21688391314 -12.36496431681 13.1358 12.6597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52889_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52889_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:46:01.28 -08:52:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.150 3761590357075170304 161.50503194159 -08.87032893114 13.1718 12.5353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52893_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52893_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:48:35.48 -10:41:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.082 3758071683643816192 162.14837947582 -10.68567335935 13.0986 12.6563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52894_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52894_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:44.79 -11:07:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.435 3760657387099265792 161.18696688036 -11.11702098354 12.9446 12.3182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52896_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52896_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:46:26.68 -10:47:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.567 3760693950156622080 161.61147240920 -10.79987058520 12.9888 12.5307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52898_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52898_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:51:47.41 -14:14:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.295 3756021330681012352 162.94840371758 -14.23426261723 12.9754 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52900_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52900_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:51:53.38 -14:13:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.215 3756020609126506496 162.97227014854 -14.23249925562 12.7437 12.2317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52902_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 52902_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 52908_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 52908_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 52909_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52909_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 52910_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52910_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:47:19.80 -10:11:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.100 3761126745421077760 161.83337446202 -10.19519382550 12.9308 12.3217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52913_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52913_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:48:14.21 -11:58:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.332 3757365964682686208 162.05912080512 -11.97074893858 12.6681 12.0148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52914_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52914_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:23.67 -13:14:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 5.557 3751135105302551808 161.10020653862 -13.24274781191 12.7222 12.1765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52916_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52916_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:48:01.85 -12:23:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 0.297 3757197743698594688 162.00762588123 -12.38476752103 12.7631 12.2350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52918_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52918_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:50.27 -13:23:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.242 3751117337022290944 161.21034744717 -13.39558427543 12.7275 12.1740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52925_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 52925_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 52929_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52929_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:47:42.48 -13:22:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.275 3756359915838190720 161.92735982525 -13.37516418439 12.8274 12.3182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52930_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52930_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:45:42.66 -14:11:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.934 3750254980604308224 161.42804552705 -14.19225984861 12.4994 11.9071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52931_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52931_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:43:52.56 -09:37:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 0.416 3761432027401099776 160.96892142934 -09.61841901321 12.7316 12.2482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52933_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52933_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:47:18.11 -13:06:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.863 3757131012791628288 161.82622738549 -13.10518414631 12.4036 11.7669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52936_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52936_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:45:57.93 -10:49:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.053 3760695427625368064 161.49123060641 -10.82527206151 12.6865 12.1557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52941_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52941_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:47:11.57 -10:29:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.856 3761083555229930240 161.79836280394 -10.48646058931 12.6828 12.1720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52944_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52944_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:49.79 -11:38:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.105 3757531303742803072 161.20716807846 -11.64360633698 12.4744 11.8156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52952_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52952_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:46:53.96 -12:51:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.087 3757155275061945728 161.72571288468 -12.85934534304 12.5881 12.1039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52953_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52953_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:43:52.91 -12:26:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.706 3757414931604714624 160.97119468057 -12.44516953572 12.4913 11.9838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52955_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52955_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:22.94 -12:32:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.308 3757411736149042176 161.09533049139 -12.53956687092 12.5106 11.9869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52956_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52956_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:52:14.10 -13:39:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.504 3756113934471348992 163.05946186382 -13.65135048624 12.6556 12.0104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52959_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52959_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:45:22.44 -10:15:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 0.315 3761147533062855424 161.34358893768 -10.25269259343 12.6911 12.3047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52961_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52961_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:51.47 -12:06:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.038 3757463069598206592 161.21426376559 -12.10438321608 12.6648 12.1731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52968_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52968_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:46:49.59 -12:05:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.165 3757268249881683328 161.70692108250 -12.08853325581 12.6062 12.1220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52969_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52969_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:46:49.82 -13:29:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 0.979 3750364278932089088 161.70747454457 -13.49702828665 12.4545 11.9982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52971_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52971_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52972_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52972_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 52973_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52973_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:46:35.95 -10:08:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.270 3761151892454472320 161.65071443912 -10.14883200303 12.6109 12.0481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52974_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52974_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:48:00.24 -13:26:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.961 3756358472729178496 162.00181704672 -13.44379557149 12.4434 11.9115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52975_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52975_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:49:26.37 -14:13:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.581 3750064112257614976 162.36084512822 -14.22661504903 12.2216 11.5186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52976_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52976_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:46:52.01 -13:34:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.791 3750346068270748032 161.71691503072 -13.58228315029 12.7603 12.2837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52984_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52984_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:13.24 -13:14:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 2.470 3751134860488855680 161.05505836208 -13.24895574736 12.2385 11.7682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52993_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52993_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:48:41.58 -12:52:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.495 3756413203496568192 162.17362757136 -12.88291437546 12.4077 11.8853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52995_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 52995_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 52996_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52996_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:45:07.56 -12:28:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.736 3757230797766815360 161.28199329446 -12.47857725826 12.3254 11.8639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52998_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 52998_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 53005_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53005_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:06.13 -08:53:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.124 3762337131628855680 161.02494977462 -08.88367239553 12.3064 11.6003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53011_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53011_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 53015_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53015_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:47:14.41 -13:19:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.287 3756375927476263424 161.80959697077 -13.32140971164 12.1648 11.5424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53023_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53023_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:50:34.95 -13:48:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.011 3756097201278694656 162.64643747138 -13.81322231156 12.1244 11.6873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53027_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53027_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53032_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53032_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53033_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53033_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:43:55.78 -11:45:12.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 53035_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53035_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:48:33.52 -13:28:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.680 3756354654503229824 162.13973853687 -13.47711995902 11.9746 11.4129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53041_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53041_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53042_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53042_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:00.39 -13:01:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.672 3751189668567086208 161.00177868380 -13.02846740457 11.8547 11.2463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53044_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53044_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:00.08 -10:42:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 5.580 3760753697446514816 160.99875597992 -10.71505543900 11.7673 11.2814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53054_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53054_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53063_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53063_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53064_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53064_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:44:13.13 -13:07:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 3.750 3751185133080845824 161.05375301863 -13.12394069938 11.2795 10.7921 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53070_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53070_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53073_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53073_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53075_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53075_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53079_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53079_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53082_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53082_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53085_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53085_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53087_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53087_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53088_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53088_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53089_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53089_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53097_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53097_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:45:47.61 -13:21:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.33, MAG_FAINT_SEARCH_LIMIT=12.31)GAIADR2_OUTPUT=# 3.583 3751115726410169856 161.44786296217 -13.35447280683 10.7586 10.2869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53098_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53098_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53101_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 53101_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 53110_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53110_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:45:38.23 -13:37:12.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53612_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53612_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53721_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 53721_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54713_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 54713_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54826_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 54826_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54846_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 54846_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54916_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 54916_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54917_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 54917_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55071_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55071_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55147_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55147_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55232_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55232_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55357_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55357_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55363_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55363_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55397_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55397_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55542_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55542_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55555_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55555_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55630_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55630_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55669_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55669_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55706_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55706_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55766_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55766_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55865_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55865_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55869_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55869_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55870_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55870_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55876_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55876_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55896_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55896_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55989_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 55989_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
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Considering the candidate 55998_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 55998_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56010_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56010_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56048_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56048_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56052_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56052_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56063_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56063_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56091_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56091_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 11:18:47.71 -06:54:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 3.759 3783985145486353792 169.69983816696 -06.90247756089 14.1584 14.0293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56092_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56092_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56097_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56097_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56100_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56100_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56131_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56131_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56145_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56145_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56191_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56191_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56227_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56227_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56238_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56238_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56242_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56242_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56255_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56255_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56276_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56276_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56277_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56277_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56283_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56283_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56285_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56285_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:48:14.07 -11:20:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56302_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56302_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56306_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56306_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56308_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56308_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56313_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56313_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56325_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56325_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56326_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56326_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56336_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56336_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56346_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56346_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56362_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56362_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56369_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56369_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56385_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56385_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56394_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56394_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56397_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56397_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56400_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56400_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56401_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56401_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56404_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56404_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56405_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56405_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56407_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56407_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56421_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 56421_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05320_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 05320_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36681_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 36681_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 11:01:55.26 -07:39:43.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06453_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 06453_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39066_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
Preparing report for the candidate 39066_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16112_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 16112_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 11:05:34.00 -11:05:21.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15171_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 15171_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 11:03:14.82 -11:18:12.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06870_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 06870_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 11:03:36.58 -13:26:04.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09759_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 09759_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 11:15:39.57 -12:35:29.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20931_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 20931_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:49:43.61 -09:51:10.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24889_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 24889_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:50:18.22 -08:53:52.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03973_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 03973_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 11:00:11.78 -14:04:56.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05497_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 05497_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:54:17.85 -13:45:26.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24735_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161
The candidate 24735_fd_Crt-01-Q2b1x1_2026-04-06_00-04-35_20.00sec_-4.90C_LIGHT_0161 did not pass the final checks
**** FOUND 10:48:49.10 -09:00:01.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 50s
Prepared the HTML report for the field Crt-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:01:55.26 -07:39:43.8
10:45:06.68 -12:45:42.2
10:48:45.03 -14:06:19.5
10:45:38.23 -13:37:11.4
10:53:28.40 -08:18:10.0
10:44:44.14 -13:39:33.4
10:44:57.83 -11:56:19.3
10:46:50.47 -12:32:58.6
10:44:46.47 -12:27:22.3
10:44:53.43 -11:19:59.2
10:45:54.96 -13:02:13.2
10:45:28.05 -13:42:45.8
10:46:08.10 -12:08:16.0
10:45:24.99 -13:53:15.4
10:47:16.10 -14:09:20.3
10:43:59.42 -12:50:09.1
10:45:47.71 -13:27:03.5
10:45:29.55 -08:52:35.4
10:46:46.63 -14:09:53.0
10:48:35.94 -14:05:31.7
10:47:11.78 -14:13:58.2
10:46:11.54 -13:47:43.8
10:44:26.22 -08:22:22.1
10:46:20.51 -12:58:47.5
10:44:30.56 -08:23:32.4
11:32:55.38 -07:10:19.1
########### Completed Crt-01-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
10:45:06.68 -12:45:42.2
10:48:45.03 -14:06:19.5
10:45:38.23 -13:37:11.4
11:01:55.26 -07:39:43.8
10:44:44.14 -13:39:33.4
10:44:57.83 -11:56:19.3
10:46:50.47 -12:32:58.6
10:44:46.47 -12:27:22.3
10:44:53.43 -11:19:59.2
10:45:54.96 -13:02:13.2
10:45:28.05 -13:42:45.8
10:46:08.10 -12:08:16.0
10:45:24.99 -13:53:15.4
10:47:16.10 -14:09:20.3
10:43:59.42 -12:50:09.1
10:45:47.71 -13:27:03.5
10:45:29.55 -08:52:35.4
10:46:46.63 -14:09:53.0
10:48:35.94 -14:05:31.7
10:47:11.78 -14:13:58.2
10:46:11.54 -13:47:43.8
10:44:26.22 -08:22:22.1
10:46:20.51 -12:58:47.5
10:44:30.56 -08:23:32.4
11:32:55.38 -07:10:19.1
10:53:28.40 -08:18:10.0
###################################################################################
10:45:06.68 -12:45:42.2 -- not an asteroid (will add it to exclusion list)
10:48:45.03 -14:06:19.5 -- not an asteroid (will add it to exclusion list)
10:45:38.23 -13:37:11.4 -- not an asteroid (will add it to exclusion list)
11:01:55.26 -07:39:43.8 -- not an asteroid (will add it to exclusion list)
10:44:44.14 -13:39:33.4 -- not an asteroid (will add it to exclusion list)
10:44:57.83 -11:56:19.3 -- not an asteroid (will add it to exclusion list)
10:46:50.47 -12:32:58.6 -- not an asteroid (will add it to exclusion list)
10:44:46.47 -12:27:22.3 -- not an asteroid (will add it to exclusion list)
10:44:53.43 -11:19:59.2 -- not an asteroid (will add it to exclusion list)
10:45:54.96 -13:02:13.2 -- not an asteroid (will add it to exclusion list)
10:45:28.05 -13:42:45.8 -- not an asteroid (will add it to exclusion list)
10:46:08.10 -12:08:16.0 -- not an asteroid (will add it to exclusion list)
10:45:24.99 -13:53:15.4 -- not an asteroid (will add it to exclusion list)
10:47:16.10 -14:09:20.3 -- not an asteroid (will add it to exclusion list)
10:43:59.42 -12:50:09.1 -- not an asteroid (will add it to exclusion list)
10:45:47.71 -13:27:03.5 -- not an asteroid (will add it to exclusion list)
10:45:29.55 -08:52:35.4 -- not an asteroid (will add it to exclusion list)
10:46:46.63 -14:09:53.0 -- not an asteroid (will add it to exclusion list)
10:48:35.94 -14:05:31.7 -- not an asteroid (will add it to exclusion list)
10:47:11.78 -14:13:58.2 -- not an asteroid (will add it to exclusion list)
10:46:11.54 -13:47:43.8 -- not an asteroid (will add it to exclusion list)
10:44:26.22 -08:22:22.1 -- not an asteroid (will add it to exclusion list)
10:46:20.51 -12:58:47.5 -- not an asteroid (will add it to exclusion list)
10:44:30.56 -08:23:32.4 -- not an asteroid (will add it to exclusion list)
11:32:55.38 -07:10:19.1 -- asteroid (will NOT add it to exclusion list)
10:53:28.40 -08:18:10.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
10:43:59.42 -12:50:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:44:26.22 -08:22:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:44:30.56 -08:23:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:44:44.14 -13:39:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:44:46.47 -12:27:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:44:53.43 -11:19:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:44:57.83 -11:56:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:06.68 -12:45:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:24.99 -13:53:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:28.05 -13:42:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:29.55 -08:52:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:38.23 -13:37:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:47.71 -13:27:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:54.96 -13:02:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:08.10 -12:08:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:11.54 -13:47:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:20.51 -12:58:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:46.63 -14:09:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:50.47 -12:32:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:11.78 -14:13:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:16.10 -14:09:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:35.94 -14:05:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:45.03 -14:06:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:53:28.40 -08:18:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:01:55.26 -07:39:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
10:43:59.42 -12:50:09.1 -- not a known variable star
10:44:26.22 -08:22:22.1 -- not a known variable star
10:44:30.56 -08:23:32.4 -- not a known variable star
10:44:44.14 -13:39:33.4 -- not a known variable star
10:44:46.47 -12:27:22.3 -- not a known variable star
10:44:53.43 -11:19:59.2 -- not a known variable star
10:44:57.83 -11:56:19.3 -- not a known variable star
10:45:06.68 -12:45:42.2 -- not a known variable star
10:45:24.99 -13:53:15.4 -- not a known variable star
10:45:28.05 -13:42:45.8 -- not a known variable star
10:45:29.55 -08:52:35.4 -- not a known variable star
10:45:38.23 -13:37:11.4 -- not a known variable star
10:45:47.71 -13:27:03.5 -- not a known variable star
10:45:54.96 -13:02:13.2 -- not a known variable star
10:46:08.10 -12:08:16.0 -- not a known variable star
10:46:11.54 -13:47:43.8 -- not a known variable star
10:46:20.51 -12:58:47.5 -- not a known variable star
10:46:46.63 -14:09:53.0 -- not a known variable star
10:46:50.47 -12:32:58.6 -- not a known variable star
10:47:11.78 -14:13:58.2 -- not a known variable star
10:47:16.10 -14:09:20.3 -- not a known variable star
10:48:35.94 -14:05:31.7 -- not a known variable star
10:48:45.03 -14:06:19.5 -- not a known variable star
10:53:28.40 -08:18:10.0 -- a known variable star
11:01:55.26 -07:39:43.8 -- a known variable star
Found 23 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
25 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
10:43:59.42 -12:50:09.1
10:44:26.22 -08:22:22.1
10:44:30.56 -08:23:32.4
10:44:44.14 -13:39:33.4
10:44:46.47 -12:27:22.3
10:44:53.43 -11:19:59.2
10:44:57.83 -11:56:19.3
10:45:06.68 -12:45:42.2
10:45:24.99 -13:53:15.4
10:45:28.05 -13:42:45.8
10:45:29.55 -08:52:35.4
10:45:38.23 -13:37:11.4
10:45:47.71 -13:27:03.5
10:45:54.96 -13:02:13.2
10:46:08.10 -12:08:16.0
10:46:11.54 -13:47:43.8
10:46:20.51 -12:58:47.5
10:46:46.63 -14:09:53.0
10:46:50.47 -12:32:58.6
10:47:11.78 -14:13:58.2
10:47:16.10 -14:09:20.3
10:48:35.94 -14:05:31.7
10:48:45.03 -14:06:19.5
10:53:28.40 -08:18:10.0
11:01:55.26 -07:39:43.8
10:45:48.23 -13:27:00.1
10:46:25.66 -09:02:45.5
10:45:12.57 -09:01:36.2
10:52:52.01 -12:21:54.3
10:46:01.28 -08:52:13.6
10:48:35.48 -10:41:09.2
10:44:44.79 -11:07:00.5
10:46:26.68 -10:47:58.4
10:51:47.41 -14:14:02.0
10:51:53.38 -14:13:58.1
10:47:19.80 -10:11:42.8
10:48:14.21 -11:58:13.4
10:44:23.67 -13:14:34.3
10:48:01.85 -12:23:05.1
10:44:50.27 -13:23:43.2
10:47:42.48 -13:22:30.4
10:45:42.66 -14:11:30.5
10:43:52.56 -09:37:06.0
10:47:18.11 -13:06:17.7
10:45:57.93 -10:49:31.9
10:47:11.57 -10:29:10.6
10:44:49.79 -11:38:37.4
10:46:53.96 -12:51:33.7
10:43:52.91 -12:26:43.4
10:44:22.94 -12:32:23.4
10:52:14.10 -13:39:04.6
10:45:22.44 -10:15:09.7
10:44:51.47 -12:06:15.0
10:46:49.59 -12:05:18.2
10:46:49.82 -13:29:48.4
10:46:35.95 -10:08:55.8
10:48:00.24 -13:26:36.9
10:49:26.37 -14:13:38.9
10:46:52.01 -13:34:55.9
10:44:13.24 -13:14:53.8
10:48:41.58 -12:52:57.8
10:45:07.56 -12:28:42.8
10:44:06.13 -08:53:01.5
10:47:14.41 -13:19:15.4
10:50:34.95 -13:48:48.6
10:43:55.78 -11:45:12.1
10:48:33.52 -13:28:37.0
10:44:00.39 -13:01:40.9
10:44:00.08 -10:42:54.1
10:44:13.13 -13:07:24.5
10:45:47.61 -13:21:13.0
11:18:47.71 -06:54:09.3
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461136.71111747 -observatory V36
23:20:29.36 -06:25:09.9 Mercury (0.3mag)
02:21:34.99 +13:51:29.9 Venus (-3.9mag)
23:49:57.46 -02:12:16.1 Mars (1.2mag)
07:08:42.59 +22:52:26.2 Jupiter (-2.2mag)
00:24:46.15 +00:21:16.4 Saturn (0.9mag)
03:45:43.55 +19:41:06.3 Uranus (5.8mag)
00:09:31.92 -00:23:39.4 Neptune (7.8mag)
20:33:14.23 -22:52:29.4 Pluto (14.5mag)
16:00:01.84 -26:12:02.5 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Apr 6 00:10 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461136.71111747:
07:08:46.05 +22:52:16.7 Io (5.7mag)
07:08:55.28 +22:51:59.6 Europa (5.8mag)
07:08:37.27 +22:52:43.8 Ganymede (5.3mag)
07:08:12.78 +22:53:17.8 Callisto (6.5mag)
07:12:25.50 +22:44:55.8 Himalia (15.3mag)
07:08:40.27 +22:52:32.8 Thebe (16.2mag)
07:12:23.22 +23:13:42.0 Elara (17.2mag)
07:06:55.49 +23:37:34.0 Pasiphae (17.3mag)
07:17:14.38 +22:49:22.4 Carme (18.4mag)
00:24:40.87 +00:21:17.5 Titan (8.8mag)
00:24:42.94 +00:21:30.5 Rhea (10.1mag)
00:24:46.68 +00:22:49.8 Iapetus (11.5mag)
00:24:47.98 +00:21:04.7 Hyperion (14.8mag)
00:26:30.37 +00:31:05.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 6 00:10 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.71111747:
14:47:23.49 -08:20:16.2 JWST
17:01:24.88 +44:55:19.4 Chandra
08:02:12.36 -38:58:00.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 6 00:10 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.71111747 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:08.21 -28:14:11.3 14.0mag P/2010 H2 (Vales)
05:00:05.88 -70:08:48.9 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:34.35 +31:22:33.9 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.73 +09:22:20.9 17.6mag C/2021 G2 (ATLAS)
23:07:21.49 +28:52:07.4 17.0mag C/2022 E2 (ATLAS)
04:18:00.85 +25:45:53.5 15.9mag C/2022 N2 (PANSTARRS)
09:01:52.06 +31:54:24.8 16.1mag C/2022 QE78 (ATLAS)
08:29:59.26 -01:13:49.6 17.3mag C/2022 R6 (PANSTARRS)
18:55:35.19 +17:41:47.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:30.37 -11:39:36.9 17.6mag P/2023 B1 (PANSTARRS)
09:12:49.50 -13:29:59.6 17.5mag C/2023 F3 (ATLAS)
21:43:29.92 +62:22:20.0 17.5mag C/2023 H5 (Lemmon)
19:26:23.97 -03:36:31.4 14.3mag C/2023 R1 (PANSTARRS)
21:42:38.53 +84:36:48.0 17.8mag C/2023 X2 (Lemmon)
06:14:31.99 +63:35:00.8 17.0mag C/2024 A1 (ATLAS)
04:51:06.72 +14:33:51.0 10.4mag C/2024 E1 (Wierzchos)
16:25:05.54 +04:46:51.6 17.4mag C/2024 G6 (ATLAS)
20:17:33.38 +12:41:18.9 14.7mag C/2024 J3 (ATLAS)
03:17:46.98 -23:55:11.2 16.4mag C/2024 T5 (ATLAS)
05:08:43.17 +47:49:46.0 17.7mag C/2025 J1 (Borisov)
14:19:01.53 +37:24:40.0 14.8mag C/2025 L1 (ATLAS)
03:10:23.79 -24:45:06.4 17.8mag C/2025 Q3 (ATLAS)
22:53:37.70 +19:50:14.0 10.1mag C/2025 R3 (PANSTARRS)
12:58:23.00 +02:23:36.4 17.5mag C/2025 Y1 (ATLAS)
01:31:22.52 +04:42:22.2 7.1mag C/2026 A1 (MAPS)
23:30:52.00 +35:14:53.4 14.3mag C/2026 B2 (Sun-Gao)
18:23:49.76 -10:13:02.8 12.4mag 10P/Tempel
15:12:52.83 +04:06:37.8 13.1mag 24P/Schaumasse
11:05:45.87 -01:51:47.1 15.7mag 29P/Schwassmann-Wachmann
17:56:46.39 -09:59:31.9 17.7mag 40P/Vaisala
10:38:52.78 -04:56:46.8 16.7mag 43P/Wolf-Harrington
01:33:34.95 +15:47:58.2 17.1mag 47P/Ashbrook-Jackson
06:53:21.89 +39:04:36.5 17.0mag 63P/Wild
23:16:20.07 -12:39:09.2 15.7mag 65P/Gunn
03:37:43.61 +17:44:42.7 15.8mag 76P/West-Kohoutek-Ikemura
00:44:07.32 +06:17:20.7 14.4mag 78P/Gehrels
22:32:36.64 -12:15:56.7 14.5mag 88P/Howell
01:43:13.48 +17:57:10.8 15.1mag 93P/Lovas
04:36:57.62 +31:43:46.2 16.3mag 123P/West-Hartley
08:17:57.02 +42:52:54.6 16.2mag 124P/Mrkos
02:18:14.83 +13:15:33.3 16.4mag 128P/Shoemaker-Holt
02:28:26.19 +13:15:22.6 17.5mag 131P/Mueller
00:35:58.80 +09:37:03.6 11.2mag 141P/Machholz
00:45:57.17 +01:12:26.1 11.3mag 141P-A/Machholz
23:36:30.64 -02:25:00.1 14.0mag 141P-D/Machholz
01:15:04.63 +02:52:20.1 17.9mag 141P-I/Machholz
00:35:11.49 -06:24:29.3 15.2mag 162P/SidingSpring
10:30:58.22 +31:30:18.8 17.8mag 164P/Christensen
06:18:27.94 +24:31:21.6 17.8mag 198P/ODAS
15:08:40.07 -01:11:35.4 17.4mag 210P/Christensen
21:08:58.69 -13:48:59.9 17.4mag 218P/LINEAR
17:12:36.87 -15:04:15.2 16.2mag 235P/LINEAR
05:13:42.02 +33:51:28.6 16.6mag 240P/NEAT
07:34:12.50 -06:17:04.7 17.6mag 242P/Spahr
15:45:55.99 +06:18:38.3 17.5mag 391P/Kowalski
07:30:55.41 +21:18:42.5 17.6mag 450P/LONEOS
05:21:56.63 +45:36:36.6 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 6 00:10 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
-rw-r--r-- 1 apache apache 5.8K Apr 6 00:10 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 6 00:10 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:34:24.360 +36:48:31.82 AT 2026huj 2026-03-20.71 20.85
07:36:21.380 +15:56:54.55 AT 2026hui 2026-03-18.71 20.7
11:53:11.050 +21:20:34.15 AT 2026huh 2026-03-17.78 21.68
11:11:02.080 +21:51:43.20 AT 2026hug 2026-03-17.78 21.19
11:58:25.850 +16:51:27.33 AT 2026huf 2026-03-17.78 21.62
07:42:32.090 +18:28:41.88 AT 2026hue 2026-03-17.76 21.39
09:40:01.520 +16:17:02.86 AT 2026hud 2026-03-17.76 20.71
09:20:25.810 +14:33:34.07 AT 2026huc 2026-03-17.76 20.65
06:44:02.780 +20:39:27.33 AT 2026hub 2026-03-18.72 20.62
13:08:33.600 +42:15:08.61 AT 2026hua 2026-03-15.75 21.43
13:21:41.610 +41:21:55.04 AT 2026htz 2026-03-15.75 21.4
13:27:29.400 +41:34:41.49 AT 2026hty 2026-03-15.75 21.81
13:19:37.170 +40:18:57.09 AT 2026htx 2026-03-15.75 21.98
13:07:58.480 +39:03:22.98 AT 2026htw 2026-03-15.75 21.29
13:33:30.740 +36:54:32.49 AT 2026htv 2026-03-15.74 21.49
13:44:31.540 +33:39:03.50 AT 2026htu 2026-03-15.74 21.57
13:38:22.690 +35:01:42.56 AT 2026htt 2026-03-15.74 21.92
13:18:28.600 +33:54:18.43 AT 2026hts 2026-03-15.74 22.06
13:14:14.650 +33:08:34.17 AT 2026htr 2026-03-15.74 21.29
13:18:12.570 +29:05:16.56 AT 2026htq 2026-03-15.74 21.89
-rw-r--r-- 1 apache apache 30K Apr 6 00:10 tns_transients_list.txt
