This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 23.2897 2461153.7897 13.12 19:06:41.04 +03:02:21.0
37.37690 -2.00018 galactic Aql Second-epoch detections are separated by 0.2" and 9.6 pix
The object was found in VSX 1" V1590 Aql
Type: M
# Max. Min./Amp. JD0 Period
13.000 I 15.400 I 2441216.00000 246.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits at 19:06:41.04 +03:02:21.0: 14.75 +/- 0.22 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits at 19:06:41.04 +03:02:21.0: 14.93 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1590 Aql,2461153.7897,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1590 Aql 20260423.2897 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 23.2897* 18 53 47.27 +02 47 02.6 13.3 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4279257581239763456,2461153.7897,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4279257581239763456 20260423.2897 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 23.2897* 18 54 32.19 +03 14 03.8 12.8 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J283.6265+03.2427,2461153.7897,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.6265+03.2427 20260423.2897 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 14039683,2461153.7897,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 14039683 20260423.2897 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190909.55+011727.4,2461153.7897,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190909.55+011727.4 20260423.2897 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185328.68+012156.8,2461153.7897,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185328.68+012156.8 20260423.2897 12.46CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4278995038480585472,2461153.7897,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4278995038480585472 20260423.2897 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 23.2897* 18 53 43.42 +04 06 11.1 12.7 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4281092185112572928,2461153.7897,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4281092185112572928 20260423.2897 12.71CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1853354+005724,2461153.7897,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1853354+005724 20260423.2897 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191159.87+040916.9,2461153.7897,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191159.87+040916.9 20260423.2897 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1902406+021201,2461153.7897,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1902406+021201 20260423.2897 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!
TCP 2026 04 23.2897* 18 57 34.85 +03 30 58.2 13.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J185734.88+033058.5,2461153.7897,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J185734.88+033058.5 20260423.2897 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J19061358+0216209,2461153.7897,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J19061358+0216209 20260423.2897 12.07CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1859293+020043,2461153.7897,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1859293+020043 20260423.2897 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1741 Aql,2461153.7897,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1741 Aql 20260423.2897 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 23.2897* 18 53 33.83 +02 40 25.5 12.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185334+0240.5,2461153.7897,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J185334+0240.5 20260423.2897 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190847.95+050451.3,2461153.7897,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190847.95+050451.3 20260423.2897 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13922798,2461153.7897,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13922798 20260423.2897 12.52CV 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 23.2897 2461153.7897 12.59 18:51:37.08 +02:08:11.0
34.85397 0.93394 galactic Aql Second-epoch detections are separated by 0.5" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4279101175713056768 | 18:51:37.11 +02:08:11.0 (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) J-Ks=1.982+/-0.028 (Very red!)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 4279101175713056768,2461153.7897,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4279101175713056768 20260423.2897 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190648.37+013013.1,2461153.7897,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190648.37+013013.1 20260423.2897 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190543.67+024432.3,2461153.7897,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190543.67+024432.3 20260423.2897 12.80CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1911453+022900,2461153.7897,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1911453+022900 20260423.2897 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J185522.09+011907.4,2461153.7897,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J185522.09+011907.4 20260423.2897 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190343+0150.8,2461153.7897,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190343+0150.8 20260423.2897 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!
TCP 2026 04 23.2897* 18 56 13.87 +02 20 01.7 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J185613.89+022001.3,2461153.7897,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J185613.89+022001.3 20260423.2897 12.45CV 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 23.2897* 18 55 17.96 +02 55 40.9 12.5 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4280752195496531968,2461153.7897,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4280752195496531968 20260423.2897 12.46CV 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: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
First image: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Last image: 2461153.79010591 23.04.2026 06:57:35.151 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.04
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): 16073
Objects passed selection criteria: 16011
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 10853.8
Average stars matched: 10572.2 (97.4064 %)
Memory usage VmPeak: 120872 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 02:24:46 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: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
First image: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Last image: 2461153.79010591 23.04.2026 06:57:35.151 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 81
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 27 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): 135164
Objects passed selection criteria: 134810
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 92604.8
Average stars matched: 88270.5 (95.3196 %)
Memory usage VmPeak: 1898636 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 02:29:25 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat to cache
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.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/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.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: 2461153.78935770
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits exists and is non-empty
Saving wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits to local_wcs_cache/
'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> 'local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits exists and is non-empty
Saving wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits to local_wcs_cache/
'wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> 'local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits exists and is non-empty
Saving wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits to local_wcs_cache/
'wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits' -> 'local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits'
wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits exists and is non-empty
Saving wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits to local_wcs_cache/
'wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits' -> 'local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits (1st reference image)
verification OK: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Image size: 942.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:43.806 +06:00:37.02 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits (1st new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
Image size: 942.7'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:26.723 +06:00:04.15 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:26.723 +06:00:04.15
Angular distance between the image centers 0.0714 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits (2nd new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
Image size: 942.7'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:29.363 +06:00:45.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:29.363 +06:00:45.13
Angular distance between the image centers 0.0599 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 18:51:26.723 +06:00:04.15
Second-epoch second image center 18:51:29.363 +06:00:45.13
Angular distance between the image centers 0.01579 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/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits &> /tmp/tmp.mEad6Q2zQQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits &> /tmp/tmp.ddS6TZgxb0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits &> /tmp/tmp.9l2KUBFxw8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits &> /tmp/tmp.XBc7KtwDZ7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
The reference image (wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits) and catalog (wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat) found
'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat' -> 'wcsmag.cat'
Read 17031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8858 to 290.8648 deg, Dec +0.6585 to +11.3165 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 274.8858 to 290.8648 deg, Dec 0.6585 to 11.3165 deg
Loaded 13648 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): 10048 out of 10700 total matches.
Matched with Tycho-2 10700 out of 17031 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.817454
a=0.000000 b=1.000000 c=22.817454
From vast_summary.log: estimated ref. image limiting mag.: -8.04
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.78
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.78
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 17031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8858 to 290.8648 deg, Dec +0.6585 to +11.3165 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 274.8858 to 290.8648 deg, Dec 0.6585 to 11.3165 deg
Loaded 13648 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): 10048 out of 10700 total matches.
Matched with Tycho-2 10700 out of 17031 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits -> calib.txt_param_ref_wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits (aperture=6.0)
Read 16916 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8731 to 290.8726 deg, Dec +0.6377 to +11.3064 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 274.8731 to 290.8726 deg, Dec 0.6377 to 11.3064 deg
Loaded 13659 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): 10039 out of 10699 total matches.
Matched with Tycho-2 10699 out of 16916 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits -> calib.txt_param_ref_wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
2.1 pix Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
3.2 pix fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
3.5 pix fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
2.1 pix wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
2.1 pix wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Limiting magnitude estimates:
14.8 mag. Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
14.8 mag. Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
13.7 mag. fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
13.7 mag. fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.2 (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.mEad6Q2zQQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> 'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1444, passed=17031
Got 17031 stars (including 15563 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 17031 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 16279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 16279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 16279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits -region wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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.ddS6TZgxb0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> 'wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1468, passed=16916
Got 16916 stars (including 15414 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
util/solve_plate_with_UCAC5 got 16916 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 16028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 16028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 16028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits -region wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.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.9l2KUBFxw8 (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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=238, passed=5439
Got 5439 stars (including 5200 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat
util/solve_plate_with_UCAC5 got 5439 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 450 to 509 (Dec 0.2 to 11.5)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 509 (Dec 0.2 to 11.5)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits -region wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.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.XBc7KtwDZ7 (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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=184, passed=4294
Got 4294 stars (including 4109 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat
util/solve_plate_with_UCAC5 got 4294 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 3966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 3964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 3964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits -region wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.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_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits'
Saving fully-calibrated image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits'
Preparing the HTML report for the field Ser-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00815_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 00815_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:02:21.04 +01:30:42.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ser-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat to cache
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Creating symlink local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.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_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits exists and is non-empty
wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits exists and is non-empty
wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits exists and is non-empty
wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits (1st reference image)
verification OK: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Image size: 942.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:43.806 +06:00:37.02 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits (1st new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
Image size: 942.7'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:26.723 +06:00:04.15 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:26.723 +06:00:04.15
Angular distance between the image centers 0.0714 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits (2nd new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 942.7'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:29.363 +06:00:45.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:29.363 +06:00:45.13
Angular distance between the image centers 0.0599 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 18:51:26.723 +06:00:04.15
Second-epoch second image center 18:51:29.363 +06:00:45.13
Angular distance between the image centers 0.01579 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/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits &> /tmp/tmp.MN5q7Kk2tk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits &> /tmp/tmp.ZHdeBVUCgq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits &> /tmp/tmp.Uv4usG8e4a
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits &> /tmp/tmp.LiActc8huf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
The reference image (wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits) and catalog (wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat) found
'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat' -> 'wcsmag.cat'
Read 147350 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8613 to 290.8654 deg, Dec +0.6327 to +11.3181 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 274.8613 to 290.8654 deg, Dec 0.6327 to 11.3181 deg
Loaded 13685 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): 9356 out of 12073 total matches.
Matched with Tycho-2 12073 out of 147350 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.635822
a=0.000000 b=1.000000 c=22.635822
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 147350 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8613 to 290.8654 deg, Dec +0.6327 to +11.3181 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 274.8613 to 290.8654 deg, Dec 0.6327 to 11.3181 deg
Loaded 13685 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): 9356 out of 12073 total matches.
Matched with Tycho-2 12073 out of 147350 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits -> calib.txt_param_ref_wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits (aperture=4.6)
Read 150239 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8731 to 290.8777 deg, Dec +0.6247 to +11.3101 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 274.8731 to 290.8777 deg, Dec 0.6247 to 11.3101 deg
Loaded 13675 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): 9302 out of 12065 total matches.
Matched with Tycho-2 12065 out of 150239 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits -> calib.txt_param_ref_wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 73 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
2.0 pix Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
2.7 pix fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
3.0 pix fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
2.1 pix wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
2.0 pix wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Limiting magnitude estimates:
14.9 mag. Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
14.9 mag. Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
13.9 mag. fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
13.8 mag. fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (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.MN5q7Kk2tk (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> 'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=17153, passed=147332
Got 147332 stars (including 129901 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 147332 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 143550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 143549 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 143550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits -region wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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.ZHdeBVUCgq (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> 'wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=17458, passed=150227
Got 150227 stars (including 132468 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
util/solve_plate_with_UCAC5 got 150227 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 146131 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 146130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 146130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits -region wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.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.Uv4usG8e4a (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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2322, passed=42574
Got 42574 stars (including 40202 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat
util/solve_plate_with_UCAC5 got 42574 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 39234 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 39234 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 39234 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits -region wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.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.LiActc8huf (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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1610, passed=32866
Got 32866 stars (including 31212 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat
util/solve_plate_with_UCAC5 got 32866 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 28855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 28856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 28856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits -region wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.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_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-56-30_20.00sec_-4.90C_LIGHTs_0133.fits
Saving fully-calibrated image wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.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_2026-04-23_CI_Ser-04-Q1b1x1_015838_TTUQ1b1x1_673091_90zaJyzM/wcs_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134.fits
Preparing the HTML report for the field Ser-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out01963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out163426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out172877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out173721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out01633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44192.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 29s
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: 17s
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Considering the candidate 172877_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 172877_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:11:08.97 +10:37:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.643 4312354599254174848 287.78691149498 +10.62603002539 13.7779 12.8357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 172891_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 172891_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:00:32.63 +04:21:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 172896_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 172896_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:11:19.41 +09:31:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 172902_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 172902_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:08:53.30 +07:32:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173268_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173268_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:56:24.58 +02:29:55.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 173405_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173405_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:20:57.47 +02:57:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173428_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173428_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:12:35.73 +10:02:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173496_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173496_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:04:51.31 +03:00:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173599_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173599_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:05:59.64 +07:21:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173667_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173667_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:20:07.13 +02:55:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173683_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173683_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:06:27.54 +07:09:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173716_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173716_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:53:53.25 +06:01:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173721_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173721_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:01:51.11 +07:49:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.223 4307095325873872384 285.46295204203 +07.83106197533 13.0279 12.2677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 173723_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173723_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:12:01.69 +04:20:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173819_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173819_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:12:45.06 +09:53:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173853_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173853_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:19:53.55 +03:39:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173857_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173857_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:11:36.83 +03:50:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173860_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 173860_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 173901_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173901_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:14:13.11 +03:41:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173949_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173949_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:16:44.84 +05:26:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173962_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 173962_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:17:31.24 +08:27:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174024_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174024_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:09:29.48 +01:27:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174027_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174027_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:02:29.17 +08:27:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174059_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174059_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:01:53.17 +07:49:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174096_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174096_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:05:04.51 +01:16:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174128_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174128_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:14:31.57 +03:52:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174159_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174159_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:15:12.11 +03:57:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174172_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174172_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:19:08.83 +06:20:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.096 4294056797293940992 289.78625668543 +06.33937582251 12.1770 10.4519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174182_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174182_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:08:25.25 +02:11:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174202_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174202_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:12:27.65 +03:42:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174212_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174212_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:19:38.28 +03:12:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174227_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174227_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:53:28.53 +01:43:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174275_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 174275_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:59:15.41 +02:26:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.001 4268674232068275456 284.81447199113 +02.44907737224 11.9680 10.2629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 17683_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 17683_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 22544_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 22544_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 26733_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 26733_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 03774_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 03774_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 04809_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 04809_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 158782_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 158782_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:21:26.46 +07:54:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158242_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 158242_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:09:43.45 +00:56:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.401 4267326196506612608 287.43180548829 +00.94680588667 11.3032 9.6864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 25219_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 25219_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:17:21.84 +03:30:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05925_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 05925_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32909_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 32909_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01633_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 01633_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18569_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 18569_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:53:08.08 +02:51:37.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01963_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 01963_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:06:34.94 +01:02:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 5.745 4267480368616703488 286.64690775967 +01.04308173556 10.9666 9.4519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33071_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 33071_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11634_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 11634_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15531_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 15531_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:58:53.29 +02:35:21.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78474_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 78474_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:22:46.44 +07:26:53.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22287_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 22287_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:14:53.00 +03:15:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.234 4292234326755913216 288.72164366737 +03.25408147977 12.1297 10.6106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25796_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 25796_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163426_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 163426_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:58:37.06 +04:49:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.178 4281599261831405056 284.65437575441 +04.82474286000 12.3849 10.8409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12055_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 12055_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09999_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 09999_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05251_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 05251_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:02:21.03 +01:30:43.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05003_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 05003_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16353_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 16353_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44192_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 44192_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13259_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 13259_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:04:50.29 +02:22:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11360_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 11360_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168687_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 168687_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:49:52.85 +01:57:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11416_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 11416_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06583_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 06583_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:53:57.45 +01:36:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05656_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 05656_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16916_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 16916_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14093_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 14093_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25734_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 25734_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 18:52:45.56 +03:30:09.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04219_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 04219_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08434_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 08434_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12977_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 12977_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25976_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 25976_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 19:11:03.59 +03:34:27.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19092_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 19092_fd_Ser-04-Q1b1x1_2026-04-23_01-57-35_20.00sec_-4.90C_LIGHTs_0134
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 47s
Prepared the HTML report for the field Ser-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:53:35.89 +00:57:15.2
19:09:09.33 +01:17:30.0
18:55:21.95 +01:19:07.4
18:53:28.65 +01:21:57.4
19:02:39.56 +01:29:15.7
19:06:48.28 +01:30:15.5
18:51:22.85 +01:29:11.4
19:03:43.17 +01:50:45.9
18:59:28.99 +02:00:38.3
18:53:54.78 +02:08:18.9
18:51:37.08 +02:08:11.0
19:02:40.03 +02:11:57.9
19:06:13.47 +02:16:21.9
18:56:13.87 +02:20:01.7
19:11:45.15 +02:29:01.9
18:53:33.83 +02:40:25.5
19:05:43.56 +02:44:33.8
19:06:41.04 +03:02:21.0
18:53:47.27 +02:47:02.6
18:55:17.96 +02:55:40.9
18:54:32.19 +03:14:03.8
18:57:34.85 +03:30:58.2
19:11:53.00 +03:38:40.0
18:53:43.42 +04:06:11.1
19:11:59.84 +04:09:17.5
19:08:47.61 +05:04:50.9
########### Completed Ser-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
19:06:41.04 +03:02:21.0
18:53:47.27 +02:47:02.6
18:54:32.19 +03:14:03.8
19:11:53.00 +03:38:40.0
19:09:09.33 +01:17:30.0
18:53:28.65 +01:21:57.4
18:51:22.85 +01:29:11.4
18:53:43.42 +04:06:11.1
18:53:35.89 +00:57:15.2
19:11:59.84 +04:09:17.5
19:02:40.03 +02:11:57.9
18:57:34.85 +03:30:58.2
19:06:13.47 +02:16:21.9
18:59:28.99 +02:00:38.3
19:02:39.56 +01:29:15.7
18:53:33.83 +02:40:25.5
19:08:47.61 +05:04:50.9
18:53:54.78 +02:08:18.9
18:51:37.08 +02:08:11.0
19:06:48.28 +01:30:15.5
19:05:43.56 +02:44:33.8
19:11:45.15 +02:29:01.9
18:55:21.95 +01:19:07.4
19:03:43.17 +01:50:45.9
18:56:13.87 +02:20:01.7
18:55:17.96 +02:55:40.9
###################################################################################
19:06:41.04 +03:02:21.0 -- not an asteroid (will add it to exclusion list)
18:53:47.27 +02:47:02.6 -- not an asteroid (will add it to exclusion list)
18:54:32.19 +03:14:03.8 -- not an asteroid (will add it to exclusion list)
19:11:53.00 +03:38:40.0 -- not an asteroid (will add it to exclusion list)
19:09:09.33 +01:17:30.0 -- not an asteroid (will add it to exclusion list)
18:53:28.65 +01:21:57.4 -- not an asteroid (will add it to exclusion list)
18:51:22.85 +01:29:11.4 -- not an asteroid (will add it to exclusion list)
18:53:43.42 +04:06:11.1 -- not an asteroid (will add it to exclusion list)
18:53:35.89 +00:57:15.2 -- not an asteroid (will add it to exclusion list)
19:11:59.84 +04:09:17.5 -- not an asteroid (will add it to exclusion list)
19:02:40.03 +02:11:57.9 -- not an asteroid (will add it to exclusion list)
18:57:34.85 +03:30:58.2 -- not an asteroid (will add it to exclusion list)
19:06:13.47 +02:16:21.9 -- not an asteroid (will add it to exclusion list)
18:59:28.99 +02:00:38.3 -- not an asteroid (will add it to exclusion list)
19:02:39.56 +01:29:15.7 -- not an asteroid (will add it to exclusion list)
18:53:33.83 +02:40:25.5 -- not an asteroid (will add it to exclusion list)
19:08:47.61 +05:04:50.9 -- not an asteroid (will add it to exclusion list)
18:53:54.78 +02:08:18.9 -- not an asteroid (will add it to exclusion list)
18:51:37.08 +02:08:11.0 -- not an asteroid (will add it to exclusion list)
19:06:48.28 +01:30:15.5 -- not an asteroid (will add it to exclusion list)
19:05:43.56 +02:44:33.8 -- not an asteroid (will add it to exclusion list)
19:11:45.15 +02:29:01.9 -- not an asteroid (will add it to exclusion list)
18:55:21.95 +01:19:07.4 -- not an asteroid (will add it to exclusion list)
19:03:43.17 +01:50:45.9 -- not an asteroid (will add it to exclusion list)
18:56:13.87 +02:20:01.7 -- not an asteroid (will add it to exclusion list)
18:55:17.96 +02:55:40.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:51:22.85 +01:29:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:37.08 +02:08:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:28.65 +01:21:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:33.83 +02:40:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:35.89 +00:57:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:43.42 +04:06:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:47.27 +02:47:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:54.78 +02:08:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:32.19 +03:14:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:17.96 +02:55:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:21.95 +01:19:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:13.87 +02:20:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:57:34.85 +03:30:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:28.99 +02:00:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:39.56 +01:29:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:40.03 +02:11:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:43.17 +01:50:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:43.56 +02:44:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:13.47 +02:16:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:41.04 +03:02:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:48.28 +01:30:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:47.61 +05:04:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:09.33 +01:17:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:45.15 +02:29:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:53.00 +03:38:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:59.84 +04:09:17.5 -- 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)
18:51:22.85 +01:29:11.4 -- a known variable star
18:51:37.08 +02:08:11.0 -- not a known variable star
18:53:28.65 +01:21:57.4 -- a known variable star
18:53:33.83 +02:40:25.5 -- a known variable star
18:53:35.89 +00:57:15.2 -- a known variable star
18:53:43.42 +04:06:11.1 -- a known variable star
18:53:47.27 +02:47:02.6 -- a known variable star
18:53:54.78 +02:08:18.9 -- a known variable star
18:54:32.19 +03:14:03.8 -- not a known variable star
18:55:17.96 +02:55:40.9 -- a known variable star
18:55:21.95 +01:19:07.4 -- a known variable star
18:56:13.87 +02:20:01.7 -- a known variable star
18:57:34.85 +03:30:58.2 -- a known variable star
18:59:28.99 +02:00:38.3 -- a known variable star
19:02:39.56 +01:29:15.7 -- a known variable star
19:02:40.03 +02:11:57.9 -- a known variable star
19:03:43.17 +01:50:45.9 -- a known variable star
19:05:43.56 +02:44:33.8 -- a known variable star
19:06:13.47 +02:16:21.9 -- a known variable star
19:06:41.04 +03:02:21.0 -- a known variable star
19:06:48.28 +01:30:15.5 -- a known variable star
19:08:47.61 +05:04:50.9 -- a known variable star
19:09:09.33 +01:17:30.0 -- a known variable star
19:11:45.15 +02:29:01.9 -- a known variable star
19:11:53.00 +03:38:40.0 -- a known variable star
19:11:59.84 +04:09:17.5 -- a known variable star
Found 2 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
26 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 ####
18:51:22.85 +01:29:11.4
18:51:37.08 +02:08:11.0
18:53:28.65 +01:21:57.4
18:53:33.83 +02:40:25.5
18:53:35.89 +00:57:15.2
18:53:43.42 +04:06:11.1
18:53:47.27 +02:47:02.6
18:53:54.78 +02:08:18.9
18:54:32.19 +03:14:03.8
18:55:17.96 +02:55:40.9
18:55:21.95 +01:19:07.4
18:56:13.87 +02:20:01.7
18:57:34.85 +03:30:58.2
18:59:28.99 +02:00:38.3
19:02:39.56 +01:29:15.7
19:02:40.03 +02:11:57.9
19:03:43.17 +01:50:45.9
19:05:43.56 +02:44:33.8
19:06:13.47 +02:16:21.9
19:06:41.04 +03:02:21.0
19:06:48.28 +01:30:15.5
19:08:47.61 +05:04:50.9
19:09:09.33 +01:17:30.0
19:11:45.15 +02:29:01.9
19:11:53.00 +03:38:40.0
19:11:59.84 +04:09:17.5
19:06:34.94 +01:02:38.3
19:09:43.45 +00:56:46.5
18:58:37.06 +04:49:25.9
19:11:08.97 +10:37:33.8
19:01:51.11 +07:49:49.6
19:19:08.83 +06:20:20.9
18:59:15.41 +02:26:57.0
19:14:53.00 +03:15:16.1
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The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461153.78935770 -observatory V36
00:48:21.30 +02:26:56.6 Mercury (-0.3mag)
03:44:46.43 +20:22:23.7 Venus (-3.9mag)
00:38:30.90 +03:07:40.5 Mars (1.2mag)
07:16:13.05 +22:40:09.2 Jupiter (-2.1mag)
00:32:23.29 +01:08:50.9 Saturn (0.9mag)
03:49:16.54 +19:52:29.8 Uranus (5.8mag)
00:11:46.31 -00:09:31.6 Neptune (7.8mag)
20:34:01.28 -22:53:07.7 Pluto (14.5mag)
07:35:00.17 +24:37:53.5 Moon (-10.1mag)
-rw-r--r-- 1 apache apache 363 Apr 23 02:24 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461153.78935770:
07:16:16.88 +22:40:03.1 Io (5.8mag)
07:16:19.67 +22:39:56.9 Europa (6.0mag)
07:16:29.84 +22:39:28.9 Ganymede (5.4mag)
07:15:43.22 +22:41:08.2 Callisto (6.6mag)
07:19:12.57 +22:24:36.5 Himalia (15.4mag)
07:16:17.41 +22:39:59.5 Thebe (16.3mag)
07:19:32.30 +22:54:52.1 Elara (17.3mag)
07:15:35.60 +23:16:20.7 Pasiphae (17.5mag)
07:24:22.42 +22:38:49.6 Carme (18.6mag)
00:32:21.97 +01:08:42.0 Titan (8.8mag)
00:32:24.89 +01:09:05.3 Rhea (10.1mag)
00:31:54.55 +01:07:51.9 Iapetus (11.5mag)
00:32:12.80 +01:08:59.2 Hyperion (14.8mag)
00:33:54.13 +01:16:50.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 23 02:24 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461153.78935770:
16:06:45.89 -20:56:56.8 JWST
19:02:45.87 +19:17:42.4 Chandra
18:34:44.36 -25:29:01.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 23 02:24 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461153.78935770 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
05:37:06.35 +30:48:09.2 18.0mag P/2009 WX51 (Catalina)
18:54:24.50 -29:13:39.4 13.8mag P/2010 H2 (Vales)
05:12:11.54 -69:19:56.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:34:09.64 +31:29:25.4 17.3mag C/2017 K2 (PANSTARRS)
17:29:26.90 +11:23:39.5 17.7mag C/2021 G2 (ATLAS)
23:11:58.34 +29:31:55.9 17.1mag C/2022 E2 (ATLAS)
04:37:49.94 +26:13:44.2 16.1mag C/2022 N2 (PANSTARRS)
09:05:19.62 +32:01:45.4 16.3mag C/2022 QE78 (ATLAS)
08:32:27.24 +00:35:20.6 17.4mag C/2022 R6 (PANSTARRS)
18:51:42.25 +19:07:44.4 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:38:07.61 -11:24:50.7 17.5mag P/2023 B1 (PANSTARRS)
09:04:40.46 -10:45:15.5 17.7mag C/2023 F3 (ATLAS)
22:00:56.27 +63:21:19.6 17.6mag C/2023 H5 (Lemmon)
19:12:01.07 -03:52:58.8 14.1mag C/2023 R1 (PANSTARRS)
21:07:00.73 +86:56:07.0 17.8mag C/2023 X2 (Lemmon)
06:21:59.41 +63:30:01.1 17.2mag C/2024 A1 (ATLAS)
05:28:19.52 +20:29:08.0 11.5mag C/2024 E1 (Wierzchos)
16:14:18.59 +07:34:22.4 17.3mag C/2024 G6 (ATLAS)
20:22:29.16 +17:17:55.4 14.5mag C/2024 J3 (ATLAS)
03:33:01.98 -21:18:26.1 16.3mag C/2024 T5 (ATLAS)
05:23:03.53 +43:32:45.6 17.7mag C/2025 J1 (Borisov)
13:09:22.62 +49:17:44.9 15.5mag C/2025 L1 (ATLAS)
03:37:11.57 -27:24:03.3 17.9mag C/2025 Q3 (ATLAS)
01:25:08.02 +12:49:25.7 7.8mag C/2025 R3 (PANSTARRS)
12:51:01.82 +03:26:00.1 17.4mag C/2025 Y1 (ATLAS)
04:16:26.78 +02:03:49.5 15.1mag C/2026 A1 (MAPS)
00:19:37.99 +38:27:48.8 14.8mag C/2026 B2 (Sun-Gao)
18:57:04.78 -09:19:17.5 11.4mag 10P/Tempel
14:50:22.16 +02:22:21.9 14.6mag 24P/Schaumasse
11:01:06.34 -01:18:34.2 15.7mag 29P/Schwassmann-Wachmann
10:37:51.72 -03:34:28.3 17.1mag 43P/Wolf-Harrington
01:59:59.69 +18:42:51.4 17.3mag 47P/Ashbrook-Jackson
07:24:35.63 +35:24:54.7 17.0mag 63P/Wild
23:38:10.92 -10:35:45.4 15.7mag 65P/Gunn
04:23:09.30 +23:39:12.9 15.9mag 76P/West-Kohoutek-Ikemura
01:21:49.54 +09:38:39.8 14.2mag 78P/Gehrels
23:24:34.81 -07:14:12.6 14.7mag 88P/Howell
02:31:23.13 +22:31:09.7 15.0mag 93P/Lovas
05:08:56.09 +32:38:45.4 16.1mag 123P/West-Hartley
08:37:33.23 +35:00:28.0 16.2mag 124P/Mrkos
02:44:35.08 +15:10:01.0 16.4mag 128P/Shoemaker-Holt
03:01:54.30 +15:20:57.8 17.5mag 131P/Mueller
02:05:05.72 +15:32:30.1 10.5mag 141P/Machholz
02:12:49.35 +07:33:51.2 10.5mag 141P-A/Machholz
00:55:07.98 +03:18:15.0 12.0mag 141P-D/Machholz
02:43:27.58 +09:17:22.2 17.9mag 141P-I/Machholz
01:22:50.14 +02:09:23.1 15.0mag 162P/SidingSpring
14:38:40.54 +00:35:15.6 17.9mag 210P/Christensen
21:58:56.88 -09:42:55.3 17.8mag 218P/LINEAR
17:17:24.53 -13:02:30.1 16.1mag 235P/LINEAR
05:50:26.27 +35:11:00.0 16.9mag 240P/NEAT
07:42:24.38 -04:25:11.8 17.8mag 242P/Spahr
22:35:09.62 -18:57:09.6 17.7mag 260P/McNaught
02:13:22.16 +22:16:42.5 17.9mag 295P/LINEAR
15:39:30.23 +07:26:18.7 17.5mag 391P/Kowalski
07:37:18.30 +21:22:19.7 17.7mag 450P/LONEOS
05:46:43.02 +44:36:24.1 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 23 02:24 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
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
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
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
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
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
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
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
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
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
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
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
-rw-r--r-- 1 apache apache 5.8K Apr 23 02:24 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 23 02:24 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:13:00.934 -11:35:38.06 AT 2026jrb 2026-04-09.42 18.3562
16:22:35.208 -07:41:50.91 AT 2026jra 2026-04-15.42 18.678
14:38:49.756 +05:59:17.55 AT 2026jqz 2026-04-10.33 20.5079
17:37:46.128 -00:10:27.29 AT 2026jqy 2026-04-15.44 19.9423
21:22:43.135 +01:34:03.91 AT 2026jqx 2026-04-15.50 19.506
20:20:49.879 -54:50:37.33 AT 2026jqw 2026-04-15.38 18.428
14:18:06.700 +18:27:11.82 AT 2026jqv 2026-04-15.09 18.593
05:54:56.359 -64:02:05.45 AT 2026jqu 2026-04-15.74 19.448
23:56:40.308 -79:35:41.95 AT 2026jqt 2026-04-15.38 18.924
04:07:29.216 -53:22:08.08 AT 2026jqs 2026-04-15.75 18.414
15:43:49.348 +30:31:32.85 AT 2026jqr 2026-04-15.07 19.396
10:01:06.186 +12:53:37.52 AT 2026jqq 2026-04-14.00 19.168
21:41:55.797 +08:42:01.92 AT 2026jqp 2026-04-15.51 19.6758
20:30:05.017 +14:09:09.48 AT 2026jqo 2026-04-13.20 19.78
18:56:45.384 +43:09:18.15 AT 2026jqn 2026-04-14.23 18.62
12:34:36.583 +07:30:35.59 AT 2026jqm 2026-04-15.29 22.3871
21:15:43.547 +02:04:36.79 AT 2026jql 2026-04-10.51 18.5787
21:17:35.104 -09:31:48.68 AT 2026jqk 2026-04-08.51 19.2234
23:17:19.653 +25:48:48.77 AT 2026jqj 2026-04-10.52 19.017
21:35:46.821 -63:54:12.77 SN 2026jqi 2026-04-15.38 18.808
-rw-r--r-- 1 apache apache 30K Apr 23 02:24 tns_transients_list.txt
