This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS
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 05 26.2227 2461186.7227 12.16 19:42:04.45 +14:51:05.4
51.93045 -4.10871 galactic Aql Second-epoch detections are separated by 1.7" and 3.8 pix
The object was found in VSX 2" ASASSN-V J194204.50+145106.8
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 13.690 V 2458646.24710 58.167136300000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:42:04.45 +14:51:05.4: 13.11 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:42:04.45 +14:51:05.4: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
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
ASASSN-V J194204.50+145106.8,2461186.7227,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194204.50+145106.8 20260526.2227 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.09 19:26:57.88 +11:14:16.9
46.98101 -2.63138 galactic Aql Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4314866497959164160 | 19:26:56.44 +11:14:24.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:26:57.88 +11:14:16.9: 13.11 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:26:57.88 +11:14:16.9: 13.19 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4314866497959164160,2461186.7227,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4314866497959164160 20260526.2227 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.27 19:27:55.05 +11:19:47.9
47.17309 -2.79328 galactic Aql Second-epoch detections are separated by 1.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4314959136164120320 | 19:27:55.07 +11:19:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.363+/-0.044 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:27:55.05 +11:19:47.9: 13.23 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:27:55.05 +11:19:47.9: 13.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4314959136164120320,2461186.7227,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4314959136164120320 20260526.2227 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.16 19:29:36.29 +12:07:40.5
48.07249 -2.77632 galactic Aql Second-epoch detections are separated by 1.6" and 3.5 pix
The object was found in VSX 5" Gaia DR3 4316141764003148800
Type: E
# Max. Min./Amp. JD0 Period
14.900 G 15.120 G 2.842740000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:29:36.29 +12:07:40.5: 13.19 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:29:36.29 +12:07:40.5: 13.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4316141764003148800,2461186.7227,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4316141764003148800 20260526.2227 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.39 19:39:02.94 +13:51:05.7
50.69674 -3.95984 galactic Aql Second-epoch detections are separated by 2.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.7511+13.8491 | 19:39:02.95 +13:51:07.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.326+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:39:02.94 +13:51:05.7: 13.48 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:39:02.94 +13:51:05.7: 13.59 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.7511+13.8491,2461186.7227,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.7511+13.8491 20260526.2227 12.39CV 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 05 26.2227 2461186.7227 11.72 19:44:32.00 +15:27:52.0
52.75868 -4.32216 galactic Aql Second-epoch detections are separated by 1.7" and 3.7 pix
The object was found in VSX 5" V1387 Aql
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 14.400 V 2455105.00000 275.000000000000 K0-K3III
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:44:32.00 +15:27:52.0: 12.80 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:44:32.00 +15:27:52.0: 12.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.03
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
V1387 Aql,2461186.7227,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1387 Aql 20260526.2227 11.72CV 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 05 26.2227 2461186.7227 12.00 19:29:57.63 +11:53:32.7
47.90688 -2.96518 galactic Aql Second-epoch detections are separated by 0.1" and 3.6 pix
The object was found in VSX 1" ASASSN-V J192957.71+115333.2
Type: SR
# Max. Min./Amp. JD0 Period
13.280 V 13.430 V 2457078.13800 38.860000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:29:57.63 +11:53:32.7: 13.01 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:29:57.63 +11:53:32.7: 12.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.04
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
ASASSN-V J192957.71+115333.2,2461186.7227,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192957.71+115333.2 20260526.2227 12.00CV 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 05 26.2227 2461186.7227 11.78 19:23:27.57 +09:44:42.7
45.25643 -2.57769 galactic Aql Second-epoch detections are separated by 2.0" and 3.4 pix
The object was found in VSX13" Gaia DR3 4308602103485669376
Type:
# Max. Min./Amp. JD0 Period
19.460 G 19.950 G 0.454101000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:23:27.57 +09:44:42.7: 12.72 +/- 0.02 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:23:27.57 +09:44:42.7: 12.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 4308602103485669376,2461186.7227,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4308602103485669376 20260526.2227 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.01 19:31:16.93 +12:00:15.7
48.16013 -3.19556 galactic Aql Second-epoch detections are separated by 0.9" and 3.6 pix
The object was found in VSX 2" ASASSN-V J193116.96+120017.3
Type: SR
# Max. Min./Amp. JD0 Period
13.270 V 13.700 V 2457174.90000 94.700000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:31:16.93 +12:00:15.7: 13.03 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:31:16.93 +12:00:15.7: 13.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.04
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
ASASSN-V J193116.96+120017.3,2461186.7227,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193116.96+120017.3 20260526.2227 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
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.19 19:22:44.52 +09:44:09.7
45.16506 -2.42601 galactic Aql Second-epoch detections are separated by 2.2" and 3.6 pix
The object was found in VSX 2" ZTF J192244.65+094409.6
Type: SR
# Max. Min./Amp. JD0 Period
12.913 r Y 0.123 r 2458304.79740 38.323017300000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:22:44.52 +09:44:09.7: 13.41 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:22:44.52 +09:44:09.7: 13.55 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
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
ZTF J192244.65+094409.6,2461186.7227,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192244.65+094409.6 20260526.2227 12.19CV 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 05 26.2227 2461186.7227 12.07 19:25:09.75 +10:47:48.5
46.38237 -2.45088 galactic Aql Second-epoch detections are separated by 2.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.2946+10.7886 | 19:25:09.75 +10:47:48.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.304+/-0.030 (F)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:25:09.75 +10:47:48.5: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:25:09.75 +10:47:48.5: 13.04 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J291.2946+10.7886,2461186.7227,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J291.2946+10.7886 20260526.2227 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
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.13 19:45:47.48 +17:14:02.4
54.44838 -3.70465 galactic Sge Second-epoch detections are separated by 2.6" and 4.0 pix
The object was found in VSX 2" ASASSN-V J194547.59+171404.2
Type: SR
# Max. Min./Amp. JD0 Period
13.440 V 13.610 V 2457320.76300 31.010000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:45:47.48 +17:14:02.4: 13.10 +/- 0.06 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:45:47.48 +17:14:02.4: 12.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.04
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
ASASSN-V J194547.59+171404.2,2461186.7227,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194547.59+171404.2 20260526.2227 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 11.94 19:40:02.77 +15:03:19.3
51.86740 -3.58190 galactic Aql Second-epoch detections are separated by 1.5" and 3.8 pix
The object was found in VSX 2" V1962 Aql
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 13.900 V 2457198.00000 31.270000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:40:02.77 +15:03:19.3: 12.91 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:40:02.77 +15:03:19.3: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
V1962 Aql,2461186.7227,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1962 Aql 20260526.2227 11.94CV 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 05 26.2227 2461186.7227 12.21 19:50:39.99 +17:50:43.6
55.56325 -4.40299 galactic Sge Second-epoch detections are separated by 0.1" and 3.7 pix
The object was found in VSX 4" ASASSN-V J195040.02+175047.2
Type: SR
# Max. Min./Amp. JD0 Period
13.500 V 13.930 V 2458271.01260 72.329151500000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:50:39.99 +17:50:43.6: 13.40 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:50:39.99 +17:50:43.6: 13.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
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
ASASSN-V J195040.02+175047.2,2461186.7227,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195040.02+175047.2 20260526.2227 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
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.09 19:28:03.41 +11:17:03.6
47.14915 -2.84503 galactic Aql Second-epoch detections are separated by 1.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:28:03.41 +11:17:03.6 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.032 (G)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:28:03.41 +11:17:03.6: 13.06 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:28:03.41 +11:17:03.6: 13.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.03
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
target,2461186.7227,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260526.2227 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.23 19:44:46.53 +17:00:50.5
54.13615 -3.60366 galactic Sge Second-epoch detections are separated by 1.8" and 3.6 pix
The object was found in VSX 5" NSVS J1944465+170055
Type: L:
# Max. Min./Amp. JD0 Period
11.061 R1 Y 0.693 R1 183.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:44:46.53 +17:00:50.5: 13.04 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:44:46.53 +17:00:50.5: 13.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
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
NSVS J1944465+170055,2461186.7227,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1944465+170055 20260526.2227 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 11.95 19:32:50.60 +11:50:33.6
48.20137 -3.60821 galactic Aql Second-epoch detections are separated by 1.0" and 3.6 pix
The object was found in VSX 1" ASASSN-V J193250.64+115034.8
Type: SRS
# Max. Min./Amp. JD0 Period
13.280 V 13.480 V 2457583.94600 24.438000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:32:50.60 +11:50:33.6: 12.82 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:32:50.60 +11:50:33.6: 12.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.04
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
ASASSN-V J193250.64+115034.8,2461186.7227,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193250.64+115034.8 20260526.2227 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2227 2461186.7227 12.20 19:39:32.59 +13:44:05.5
50.65331 -4.12152 galactic Aql Second-epoch detections are separated by 1.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.8857+13.7353 | 19:39:32.58 +13:44:07.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.229+/-0.024 (M)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:39:32.59 +13:44:05.5: 13.24 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:39:32.59 +13:44:05.5: 13.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.8857+13.7353,2461186.7227,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.8857+13.7353 20260526.2227 12.20CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461125.98066250 26.03.2026 11:31:59.240 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
First image: 2461125.98066250 26.03.2026 11:31:59.240 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
Last image: 2461186.72290999 26.05.2026 05:20:49.423 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
JD time system (TT/UTC/UNKNOWN): UTC
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: 4 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): 11768
Objects passed selection criteria: 11720
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 8785
Average stars matched: 8720.75 (99.2686 %)
Memory usage VmPeak: 121212 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 26 00:25:45 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: 2461125.98066250 26.03.2026 11:31:59.240 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
First image: 2461125.98066250 26.03.2026 11:31:59.240 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
Last image: 2461186.72290999 26.05.2026 05:20:49.423 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 85
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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: 29 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): 125953
Objects passed selection criteria: 125577
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: 94526.2
Average stars matched: 93155 (98.5493 %)
Memory usage VmPeak: 1985640 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 26 00:30:36 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat to cache
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.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/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.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: 2461186.72246128
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits exists and is non-empty
Saving wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits to local_wcs_cache/
'wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits' -> 'local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits'
wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits exists and is non-empty
Saving wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits to local_wcs_cache/
'wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits' -> 'local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits'
wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits'
wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits (1st reference image)
verification OK: wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
Image size: 937.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:33:21.461 +13:59:51.97 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits (1st new image)
verification OK: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
Image size: 938.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:33:24.470 +14:01:33.09 J2000 4789.000 3195.000
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###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:21.461 +13:59:51.97
Second-epoch image center 19:33:24.470 +14:01:33.09
Angular distance between the image centers 0.0306 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits (2nd new image)
verification OK: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
Image size: 938.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:33:24.448 +14:01:11.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:21.461 +13:59:51.97
Second-epoch image center 19:33:24.448 +14:01:11.31
Angular distance between the image centers 0.0251 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 19:33:24.470 +14:01:33.09
Second-epoch second image center 19:33:24.448 +14:01:11.31
Angular distance between the image centers 0.00605 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/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits &> /tmp/tmp.jklQShtpY4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits &> /tmp/tmp.ByaoiAbguY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits &> /tmp/tmp.MgISUZuMCN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits &> /tmp/tmp.YBU845GSkb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.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_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits and wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits and wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
Found non-empty wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits and wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
The reference image (wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits) and catalog (wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat) found
'wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat' -> 'wcsmag.cat'
Read 25408 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 285.1378 to 301.6501 deg, Dec +8.5927 to +19.2728 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 285.1378 to 301.6501 deg, Dec 8.5927 to 19.2728 deg
Loaded 19079 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): 13344 out of 14515 total matches.
Matched with Tycho-2 14515 out of 25408 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.889300
a=0.000000 b=1.000000 c=22.889300
From vast_summary.log: estimated ref. image limiting mag.: -8.04
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.85
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.85
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 25408 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 285.1378 to 301.6501 deg, Dec +8.5927 to +19.2728 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 285.1378 to 301.6501 deg, Dec 8.5927 to 19.2728 deg
Loaded 19079 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): 13344 out of 14515 total matches.
Matched with Tycho-2 14515 out of 25408 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits:
Forced-photometry filter: calibrated wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits -> calib.txt_param_ref_wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits (aperture=6.3)
Read 16709 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 285.0250 to 301.4963 deg, Dec +8.5594 to +19.2989 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 285.0250 to 301.4963 deg, Dec 8.5594 to 19.2989 deg
Loaded 19060 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): 11500 out of 12092 total matches.
Matched with Tycho-2 12092 out of 16709 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits:
Forced-photometry filter: calibrated wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits -> calib.txt_param_ref_wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
2.5 pix Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
2.5 pix fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
2.5 pix fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
2.4 pix wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
2.5 pix wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
Limiting magnitude estimates:
14.8 mag. Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
14.4 mag. Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
12.1 mag. fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
12.1 mag. fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
All-image limiting magnitude estimate: 12.1 (SNR ) 10.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jklQShtpY4 (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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits' -> 'wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
WCS-calibrated image found: wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
Checking if the catalog wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
WCS catalog name: wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2547, passed=25408
Got 25408 stars (including 22836 good ones) from the SExtractor catalog wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
util/solve_plate_with_UCAC5 got 25408 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 24686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 24688 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 24688 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits N_match=967 sigma_overall_arcsec=0.688 sigma_q1_arcsec=0.491 sigma_q2_arcsec=0.828 sigma_q3_arcsec=0.656 sigma_q4_arcsec=0.751 n_q1=199 n_q2=324 n_q3=178 n_q4=266 worst_quadrant_to_overall_ratio=1.204
The image catalog is written to wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits -region wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.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.ByaoiAbguY (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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits' -> 'wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
WCS-calibrated image found: wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
Checking if the catalog wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
WCS catalog name: wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1328, passed=16709
Got 16709 stars (including 15364 good ones) from the SExtractor catalog wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 16709 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 16482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 16486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 16486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits N_match=964 sigma_overall_arcsec=0.637 sigma_q1_arcsec=0.529 sigma_q2_arcsec=0.685 sigma_q3_arcsec=0.584 sigma_q4_arcsec=0.740 n_q1=204 n_q2=293 n_q3=200 n_q4=267 worst_quadrant_to_overall_ratio=1.161
The image catalog is written to wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits -region wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.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.MgISUZuMCN (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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=185, passed=3568
Got 3568 stars (including 3379 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat
util/solve_plate_with_UCAC5 got 3568 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 3445 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 3450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 3451 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits N_match=954 sigma_overall_arcsec=0.869 sigma_q1_arcsec=0.684 sigma_q2_arcsec=0.861 sigma_q3_arcsec=0.663 sigma_q4_arcsec=1.082 n_q1=210 n_q2=256 n_q3=122 n_q4=366 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits -region wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.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.YBU845GSkb (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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=185, passed=3485
Got 3485 stars (including 3297 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat
util/solve_plate_with_UCAC5 got 3485 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 3374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 3378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 3378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits N_match=957 sigma_overall_arcsec=0.807 sigma_q1_arcsec=0.686 sigma_q2_arcsec=0.795 sigma_q3_arcsec=0.606 sigma_q4_arcsec=1.026 n_q1=202 n_q2=267 n_q3=124 n_q4=364 worst_quadrant_to_overall_ratio=1.271
The image catalog is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits -region wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits sigma_overall=0.688 worst_q_ratio=1.204
ref2=Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits sigma_overall=0.637 worst_q_ratio=1.161
new1=fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits sigma_overall=0.869 worst_q_ratio=1.245
new2=fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits sigma_overall=0.807 worst_q_ratio=1.271
reference average sigma_overall=0.6625 worst_q_ratio=1.1825
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705_astrometric_residuals.png (967 matched stars from wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107_astrometric_residuals.png (964 matched stars from wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150_astrometric_residuals.png (954 matched stars from wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151_astrometric_residuals.png (957 matched stars from wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits'
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits'
Preparing the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat to cache
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
Creating symlink local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.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_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits exists and is non-empty
wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits exists and is non-empty
wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits exists and is non-empty
wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits (1st reference image)
verification OK: wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
Image size: 937.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:33:21.461 +13:59:51.97 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits (1st new image)
verification OK: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
Image size: 938.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:33:24.470 +14:01:33.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:21.461 +13:59:51.97
Second-epoch image center 19:33:24.470 +14:01:33.09
Angular distance between the image centers 0.0306 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits (2nd new image)
verification OK: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
Image size: 938.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:33:24.448 +14:01:11.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:21.461 +13:59:51.97
Second-epoch image center 19:33:24.448 +14:01:11.31
Angular distance between the image centers 0.0251 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 19:33:24.470 +14:01:33.09
Second-epoch second image center 19:33:24.448 +14:01:11.31
Angular distance between the image centers 0.00605 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/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits &> /tmp/tmp.2nWcQWu7n3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits &> /tmp/tmp.2SZtUDfUCS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits &> /tmp/tmp.7ImZNXrCJm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits &> /tmp/tmp.VUZQbprSt6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.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_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits and wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits and wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
Found non-empty wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits and wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
The reference image (wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits) and catalog (wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat) found
'wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat' -> 'wcsmag.cat'
Read 234032 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 285.1334 to 301.6605 deg, Dec +8.5812 to +19.2728 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 285.1334 to 301.6605 deg, Dec 8.5812 to 19.2728 deg
Loaded 19113 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): 10706 out of 15949 total matches.
Matched with Tycho-2 15949 out of 234032 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.701650
a=0.000000 b=1.000000 c=22.701650
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 234032 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 285.1334 to 301.6605 deg, Dec +8.5812 to +19.2728 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 285.1334 to 301.6605 deg, Dec 8.5812 to 19.2728 deg
Loaded 19113 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): 10706 out of 15949 total matches.
Matched with Tycho-2 15949 out of 234032 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits:
Forced-photometry filter: calibrated wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits -> calib.txt_param_ref_wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits (aperture=4.6)
Read 170508 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.9798 to 301.5100 deg, Dec +8.5332 to +19.2999 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 284.9798 to 301.5100 deg, Dec 8.5332 to 19.2999 deg
Loaded 19158 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): 12465 out of 16173 total matches.
Matched with Tycho-2 16173 out of 170508 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits:
Forced-photometry filter: calibrated wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits -> calib.txt_param_ref_wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 64 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
2.1 pix Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
2.2 pix fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
2.2 pix fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
2.2 pix wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
2.1 pix wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
Limiting magnitude estimates:
15.0 mag. Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
14.6 mag. Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
12.8 mag. fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
12.8 mag. fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 12.5 (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.2nWcQWu7n3 (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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits' -> 'wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
WCS-calibrated image found: wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
Checking if the catalog wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits
WCS catalog name: wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=40563, passed=233987
Got 233987 stars (including 193166 good ones) from the SExtractor catalog wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat
util/solve_plate_with_UCAC5 got 233987 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 230602 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 230599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 230513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 976 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits N_match=976 sigma_overall_arcsec=0.659 sigma_q1_arcsec=0.498 sigma_q2_arcsec=0.770 sigma_q3_arcsec=0.627 sigma_q4_arcsec=0.785 n_q1=223 n_q2=304 n_q3=205 n_q4=244 worst_quadrant_to_overall_ratio=1.191
The image catalog is written to wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits -region wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.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.2SZtUDfUCS (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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits' -> 'wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
WCS-calibrated image found: wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
Checking if the catalog wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits
WCS catalog name: wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=20948, passed=170471
Got 170471 stars (including 149337 good ones) from the SExtractor catalog wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 170471 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 168884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 168881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 168879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits N_match=972 sigma_overall_arcsec=0.657 sigma_q1_arcsec=0.609 sigma_q2_arcsec=0.755 sigma_q3_arcsec=0.615 sigma_q4_arcsec=0.726 n_q1=213 n_q2=295 n_q3=192 n_q4=272 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits -region wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.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.7ImZNXrCJm (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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1846, passed=42487
Got 42487 stars (including 40600 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat
util/solve_plate_with_UCAC5 got 42487 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 41692 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 41691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 41691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits N_match=955 sigma_overall_arcsec=0.802 sigma_q1_arcsec=0.681 sigma_q2_arcsec=0.819 sigma_q3_arcsec=0.635 sigma_q4_arcsec=1.015 n_q1=232 n_q2=224 n_q3=140 n_q4=359 worst_quadrant_to_overall_ratio=1.266
The image catalog is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits -region wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.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.VUZQbprSt6 (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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1912, passed=41504
Got 41504 stars (including 39565 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat
util/solve_plate_with_UCAC5 got 41504 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 40678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 40674 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 40674 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits N_match=959 sigma_overall_arcsec=0.774 sigma_q1_arcsec=0.651 sigma_q2_arcsec=0.755 sigma_q3_arcsec=0.565 sigma_q4_arcsec=1.012 n_q1=225 n_q2=241 n_q3=136 n_q4=357 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits -region wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-10_20.00sec_5.00C_LIGHT_0150.fits
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.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_2026-05-26_CI_Aql-01-Q2b1x1_002252_TTUQ2b1x1_2644488_J94MLABS/wcs_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151.fits
Preparing the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:16:07.91 +14:46:02.5: 11.35 +/- 0.01 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:49:50.92 +18:08:45.1: 12.55 +/- 0.02 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:45:28.37 +16:44:08.7: 12.99 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:07:48.31 +13:09:38.4: 10.85 +/- 0.01 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:39:45.73 +16:47:02.0: 11.74 +/- 0.01 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:49:50.92 +18:08:45.1: 12.37 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:16:07.91 +14:46:02.5: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Forced photometry reference-image weighted average: 11.35 +/- 0.01
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:45:28.37 +16:44:08.7: 13.01 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 19:49:50.92 +18:08:45.1: ref_mag=12.48 +/- 0.02 new_mean_mag=12.0989 delta=0.38 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:16:07.91 +14:46:02.5: ref_mag=11.35 +/- 0.01 new_mean_mag=11.7514 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:07:48.31 +13:09:38.4: 10.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Forced photometry filter REJECTED candidate at 19:45:28.37 +16:44:08.7: ref_mag=13.00 +/- 0.03 new_mean_mag=12.6001 delta=0.40 (need > 0.90)
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry filter REJECTED candidate at 19:07:48.31 +13:09:38.4: ref_mag=10.83 +/- 0.00 new_mean_mag=11.0698 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:06:45.26 +13:32:35.4: 11.58 +/- 0.01 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:36:21.74 +15:52:10.4: 12.62 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:39:45.73 +16:47:02.0: 11.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry filter REJECTED candidate at 19:39:45.73 +16:47:02.0: ref_mag=11.75 +/- 0.01 new_mean_mag=11.6675 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:06:45.26 +13:32:35.4: 11.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Forced photometry filter REJECTED candidate at 19:06:45.26 +13:32:35.4: ref_mag=11.60 +/- 0.01 new_mean_mag=11.5413 delta=0.06 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:36:21.74 +15:52:10.4: 12.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.03
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:37:35.96 +17:26:44.1: 12.53 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 19:36:21.74 +15:52:10.4: ref_mag=12.63 +/- 0.03 new_mean_mag=12.4418 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:37:35.96 +17:26:44.1: 12.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Forced photometry filter REJECTED candidate at 19:37:35.96 +17:26:44.1: ref_mag=12.55 +/- 0.02 new_mean_mag=12.7904 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:42:04.45 +14:51:05.4: 13.11 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:26:57.88 +11:14:16.9: 13.11 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:27:55.05 +11:19:47.9: 13.23 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:26:57.88 +11:14:16.9: 13.19 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:42:04.45 +14:51:05.4: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Forced photometry filter KEPT candidate at 19:26:57.88 +11:14:16.9: ref_mag=13.13 +/- 0.03 new_mean_mag=12.0747 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter KEPT candidate at 19:42:04.45 +14:51:05.4: ref_mag=13.08 +/- 0.03 new_mean_mag=12.1571 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:29:36.29 +12:07:40.5: 13.19 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:48:20.31 +17:20:48.4: 13.15 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:27:55.05 +11:19:47.9: 13.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry filter KEPT candidate at 19:27:55.05 +11:19:47.9: ref_mag=13.26 +/- 0.03 new_mean_mag=12.2437 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:39:02.94 +13:51:05.7: 13.48 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:44:32.00 +15:27:52.0: 12.80 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:29:36.29 +12:07:40.5: 13.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:48:20.31 +17:20:48.4: 12.98 +/- 0.05 detection
Forced photometry filter KEPT candidate at 19:29:36.29 +12:07:40.5: ref_mag=13.19 +/- 0.03 new_mean_mag=12.1662 delta=1.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter REJECTED candidate at 19:48:20.31 +17:20:48.4: ref_mag=13.08 +/- 0.03 new_mean_mag=12.1782 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:42:21.49 +15:28:58.3: 12.65 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:44:32.00 +15:27:52.0: 12.83 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:39:02.94 +13:51:05.7: 13.59 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.03
Forced photometry filter KEPT candidate at 19:44:32.00 +15:27:52.0: ref_mag=12.81 +/- 0.03 new_mean_mag=11.7195 delta=1.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry filter KEPT candidate at 19:39:02.94 +13:51:05.7: ref_mag=13.51 +/- 0.04 new_mean_mag=12.3934 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:29:57.63 +11:53:32.7: 13.01 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:42:21.49 +15:28:58.3: 12.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter REJECTED candidate at 19:42:21.49 +15:28:58.3: ref_mag=12.65 +/- 0.02 new_mean_mag=12.0458 delta=0.60 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:23:27.57 +09:44:42.7: 12.72 +/- 0.02 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:29:57.63 +11:53:32.7: 12.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.04
Forced photometry filter KEPT candidate at 19:29:57.63 +11:53:32.7: ref_mag=12.97 +/- 0.04 new_mean_mag=12.0006 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:23:27.57 +09:44:42.7: 12.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter KEPT candidate at 19:23:27.57 +09:44:42.7: ref_mag=12.72 +/- 0.02 new_mean_mag=11.7704 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:31:16.93 +12:00:15.7: 13.03 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:31:16.93 +12:00:15.7: 13.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Forced photometry filter KEPT candidate at 19:31:16.93 +12:00:15.7: ref_mag=13.08 +/- 0.04 new_mean_mag=11.9508 delta=1.13 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:22:44.52 +09:44:09.7: 13.41 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:22:44.52 +09:44:09.7: 13.55 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Forced photometry filter KEPT candidate at 19:22:44.52 +09:44:09.7: ref_mag=13.44 +/- 0.04 new_mean_mag=12.1822 delta=1.26 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:25:09.75 +10:47:48.5: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:25:09.75 +10:47:48.5: 13.04 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 19:25:09.75 +10:47:48.5: ref_mag=13.00 +/- 0.02 new_mean_mag=12.0484 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:45:47.48 +17:14:02.4: 13.10 +/- 0.06 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:40:02.77 +15:03:19.3: 12.91 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:46:15.71 +17:22:10.7: 13.07 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:45:47.48 +17:14:02.4: 12.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.04
Forced photometry filter KEPT candidate at 19:45:47.48 +17:14:02.4: ref_mag=13.02 +/- 0.04 new_mean_mag=12.0993 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:40:02.77 +15:03:19.3: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter KEPT candidate at 19:40:02.77 +15:03:19.3: ref_mag=12.90 +/- 0.02 new_mean_mag=11.9193 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:46:15.71 +17:22:10.7: 12.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Forced photometry filter REJECTED candidate at 19:46:15.71 +17:22:10.7: ref_mag=13.03 +/- 0.03 new_mean_mag=12.1483 delta=0.88 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:50:39.99 +17:50:43.6: 13.40 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:28:03.41 +11:17:03.6: 13.06 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:44:46.53 +17:00:50.5: 13.04 +/- 0.04 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:50:39.99 +17:50:43.6: 13.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Forced photometry filter KEPT candidate at 19:50:39.99 +17:50:43.6: ref_mag=13.27 +/- 0.04 new_mean_mag=12.1880 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:28:03.41 +11:17:03.6: 13.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Forced photometry filter KEPT candidate at 19:28:03.41 +11:17:03.6: ref_mag=13.05 +/- 0.03 new_mean_mag=12.0846 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:44:46.53 +17:00:50.5: 13.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Forced photometry filter KEPT candidate at 19:44:46.53 +17:00:50.5: ref_mag=13.09 +/- 0.03 new_mean_mag=12.1666 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:32:50.60 +11:50:33.6: 12.82 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:32:50.60 +11:50:33.6: 12.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.04
Forced photometry filter KEPT candidate at 19:32:50.60 +11:50:33.6: ref_mag=12.85 +/- 0.04 new_mean_mag=11.9076 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:34:37.97 +11:29:30.9: 12.47 +/- 0.03 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:34:37.97 +11:29:30.9: 12.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Forced photometry filter REJECTED candidate at 19:34:37.97 +11:29:30.9: ref_mag=12.43 +/- 0.02 new_mean_mag=12.0982 delta=0.33 (need > 0.90)
Forced photometry on wcs_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits at 19:39:32.59 +13:44:05.5: 13.24 +/- 0.05 detection
Forced photometry on wcs_Aql-01-Q2b1x1_2026-04-18_03-10-46_20.00sec_-4.90C_LIGHT_0107.fits at 19:39:32.59 +13:44:05.5: 13.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.04
Forced photometry filter KEPT candidate at 19:39:32.59 +13:44:05.5: ref_mag=13.26 +/- 0.04 new_mean_mag=12.1746 delta=1.08 (need > 0.90)
Adding exclusion_list_local.txt__out108518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66966.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
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: 10s
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Considering the candidate 249375_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249375_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 249376_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249376_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:41:21.00 +14:52:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249388_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249388_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:42:07.15 +17:51:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249389_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249389_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 249390_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249390_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:50:51.03 +18:09:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249391_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249391_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:30:47.67 +17:20:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249393_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249393_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 249396_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249396_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 249405_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249405_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 249406_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249406_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 249412_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249412_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 249414_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249414_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 249415_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249415_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 249416_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249416_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:25:00.06 +11:59:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249418_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249418_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:05:16.92 +17:49:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249419_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249419_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:42:38.78 +11:48:17.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 249423_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249423_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:26:04.73 +10:23:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249425_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249425_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 249430_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249430_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:29:36.78 +12:23:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249431_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249431_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:39:37.62 +16:47:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249444_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249444_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 249445_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249445_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:40:55.20 +14:08:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249447_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249447_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:36:08.93 +12:08:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249450_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249450_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:24:14.72 +16:56:11.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 249455_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249455_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:41:20.43 +14:52:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249456_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249456_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:41:28.68 +17:09:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249457_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249457_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:05:35.27 +13:52:24.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 249460_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249460_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 249461_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 249461_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:19:51.12 +14:43:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55640_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 55640_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:48:22.96 +11:31:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57178_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 57178_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:32:03.17 +11:43:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136801_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 136801_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 46021_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 46021_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 175577_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 175577_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:38:49.11 +16:28:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192352_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 192352_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:44:57.24 +17:08:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194994_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 194994_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:45:43.32 +17:00:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47976_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 47976_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 221231_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 221231_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:50:37.25 +18:05:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66966_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 66966_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 187082_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 187082_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 191039_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 191039_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:47:34.69 +17:08:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111172_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 111172_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 152582_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 152582_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 28707_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 28707_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:44:27.28 +10:18:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152290_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 152290_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 61196_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 61196_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 17613_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 17613_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 63968_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 63968_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 22543_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 22543_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:47:35.78 +09:56:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17313_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 17313_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 37138_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 37138_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 97100_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 97100_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:50:54.77 +13:13:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190120_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 190120_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 141809_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 141809_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 187386_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 187386_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
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Considering the candidate 144892_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 144892_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:43:04.54 +15:11:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226292_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 226292_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 78721_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 78721_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:32:10.20 +12:33:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47083_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 47083_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 195043_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 195043_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 60050_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
Preparing report for the candidate 60050_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
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Considering the candidate 108898_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 108898_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
**** FOUND 19:42:07.34 +13:44:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51865_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151
The candidate 51865_fd_Aql-01-Q2b1x1_2026-05-26_00-20-49_20.00sec_5.00C_LIGHT_0151 did not pass the final checks
