This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 09.2023 2461292.7023 9.35 19:15:54.61 -04:04:03.1
32.08545 -7.29382 galactic Aql Second-epoch detections are separated by 1.3" and 8.6 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 | ATO J288.9902-04.0680 | 19:15:54.71 -04:04:02.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.874+/-0.032 (M)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:54.61 -04:04:03.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:54.61 -04:04:03.1: 10.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J288.9902-04.0680,2461292.7023,9.35,0.05,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 J288.9902-04.0680 20260909.2023 9.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2023 2461292.7023 9.36 19:16:54.66 -04:02:54.7
32.21624 -7.50790 galactic Aql Second-epoch detections are separated by 0.2" and 8.6 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 | ATO J289.2314-04.0581 | 19:16:54.61 -04:02:54.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.151+/-0.035 (F)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:54.66 -04:02:54.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:54.66 -04:02:54.7: 10.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J289.2314-04.0581,2461292.7023,9.36,0.05,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 J289.2314-04.0581 20260909.2023 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2023 2461292.7023 9.39 19:16:34.45 -03:52:20.1
32.33654 -7.35330 galactic Aql Second-epoch detections are separated by 0.1" and 8.6 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 | ATO J289.1367-03.8737 | 19:16:34.42 -03:52:20.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.150+/-0.032 (F)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:34.45 -03:52:20.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:34.45 -03:52:20.1: 10.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J289.1367-03.8737,2461292.7023,9.39,0.05,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 J289.1367-03.8737 20260909.2023 9.39CV 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 09 09.2023 2461292.7023 9.37 19:16:34.59 +00:35:20.0
36.33246 -5.32088 galactic Aql Second-epoch detections are separated by 1.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4264438947672244864 | 19:16:34.49 +00:35:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:34.59 +00:35:20.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:34.59 +00:35:20.0: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
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 4264438947672244864,2461292.7023,9.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4264438947672244864 20260909.2023 9.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2023 2461292.7023 9.40 19:16:24.37 +00:29:35.6
36.22746 -5.32694 galactic Aql Second-epoch detections are separated by 2.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J289.0955+00.4928 | 19:16:24.41 +00:29:35.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.413+/-0.035 (G)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:24.37 +00:29:35.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:24.37 +00:29:35.6: 10.57 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
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 J289.0955+00.4928,2461292.7023,9.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.0955+00.4928 20260909.2023 9.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2023 2461292.7023 9.13 19:18:42.23 -01:39:39.8
34.56517 -6.82316 galactic Aql Second-epoch detections are separated by 0.3" and 8.6 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 | ATO J289.6848-01.6565 | 19:18:42.21 -01:39:39.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.663+/-0.040 (K)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:18:42.23 -01:39:39.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:18:42.23 -01:39:39.8: 10.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.00
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 J289.6848-01.6565,2461292.7023,9.13,0.05,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
ATO J289.6848-01.6565 20260909.2023 9.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2023 2461292.7023 9.18 19:16:03.61 -02:38:13.4
33.38737 -6.67920 galactic Aql Second-epoch detections are separated by 1.2" and 8.6 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 4261135946006494592 | 19:16:03.49 -02:38:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:03.61 -02:38:13.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:03.61 -02:38:13.4: 10.37 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.37 +/- 0.00
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 4261135946006494592,2461292.7023,9.18,0.05,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 4261135946006494592 20260909.2023 9.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2023 2461292.7023 8.92 19:15:51.79 -04:10:10.0
31.98844 -7.32940 galactic Aql Second-epoch detections are separated by 1.0" and 8.6 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 | ATO J288.9584-04.1753 | 19:15:51.79 -04:10:09.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.168+/-0.031 (F)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:51.79 -04:10:10.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:51.79 -04:10:10.0: 10.34 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.34 +/- 0.00
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 J288.9584-04.1753,2461292.7023,8.92,0.05,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 J288.9584-04.1753 20260909.2023 8.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2023 2461292.7023 9.00 19:17:17.51 -02:32:12.5
33.61804 -6.90769 galactic Aql Second-epoch detections are separated by 0.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4261149243226074496 | 19:17:17.46 -02:32:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1986SAAOC..10...27K KK 881-101 J-Ks=0.214+/-0.037 (F)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:17:17.51 -02:32:12.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:17:17.51 -02:32:12.5: 10.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.24 +/- 0.00
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 4261149243226074496,2461292.7023,9.00,0.05,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
Gaia DR3 4261149243226074496 20260909.2023 9.00CV 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 09 09.2023 2461292.7023 8.77 19:15:24.68 -04:04:46.3
32.01801 -7.18827 galactic Aql Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4212465406659671808 | 19:15:24.67 -04:04:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.364+/-0.031 (G)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:24.68 -04:04:46.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:24.68 -04:04:46.3: 10.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.02 +/- 0.00
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 4212465406659671808,2461292.7023,8.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4212465406659671808 20260909.2023 8.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2023 2461292.7023 8.46 19:15:31.97 -04:10:03.8
31.95249 -7.25514 galactic Aql Second-epoch detections are separated by 0.8" and 8.6 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 | ATO J288.8800-04.1605 | 19:15:31.95 -04:10:02.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.163+/-0.041 (F)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:31.97 -04:10:03.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:31.97 -04:10:03.8: 9.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.58 +/- 0.00
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 J288.8800-04.1605,2461292.7023,8.46,0.05,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 J288.8800-04.1605 20260909.2023 8.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461229.77187336 08.07.2026 06:31:19.858 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
First image: 2461229.77187336 08.07.2026 06:31:19.858 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
Last image: 2461292.70260546 09.09.2026 04:51:35.112 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 139
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.91
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: 7 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 8914
Objects passed selection criteria: 8888
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 6520
Average stars matched: 4662 (71.5031 %)
Memory usage VmPeak: 237316 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 8 23:58:32 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 3
Ref. image: 2461229.77187336 08.07.2026 06:31:19.858 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
First image: 2461229.77187336 08.07.2026 06:31:19.858 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
Last image: 2461292.70260546 09.09.2026 04:51:35.112 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
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: 25 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 100992
Objects passed selection criteria: 100685
Measurements per detected object (mean, median, min, max): 2.0 2.0 2 3
Measurements per selected object (mean, median, min, max): 2.0 2.0 2 3
Average stars detected per image: 94344.3
Average stars matched: 69726.7 (73.9066 %)
Memory usage VmPeak: 520356 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Sep 9 00:00:44 CDT 2026
Host name: tau
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.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-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.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: 2461292.70206325
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-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits exists and is non-empty
wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits (1st reference image)
verification OK: wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
Image size: 937.5'x624.4' 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: 18:51:26.142 -01:59:36.27 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-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits (1st new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
Image size: 937.2'x624.1' 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: 18:51:54.292 -01:57:03.70 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 18:51:26.142 -01:59:36.27
Second-epoch image center 18:51:54.292 -01:57:03.70
Angular distance between the image centers 0.1246 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
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###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits (2nd new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
Image size: 937.3'x624.1' 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: 18:51:52.291 -01:56:23.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:26.142 -01:59:36.27
Second-epoch image center 18:51:52.291 -01:56:23.98
Angular distance between the image centers 0.1213 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:54.292 -01:57:03.70
Second-epoch second image center 18:51:52.291 -01:56:23.98
Angular distance between the image centers 0.01383 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits &> /tmp/tmp.VqRTQDlevZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits &> /tmp/tmp.YpO0obEgax
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits &> /tmp/tmp.t9UETYjPjX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits &> /tmp/tmp.vcNWYWj0av
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.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-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits and wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits and wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat
Found non-empty wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits and wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat
The reference image (wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat) found
'wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat' -> 'wcsmag.cat'
Read 12714 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 275.0067 to 290.7479 deg, Dec -7.2611 to +3.2758 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 275.0067 to 290.7479 deg, Dec -7.2611 to 3.2758 deg
Loaded 9411 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): 6787 out of 7189 total matches.
Matched with Tycho-2 7189 out of 12714 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.588700
a=0.000000 b=1.000000 c=22.588700
From vast_summary.log: estimated ref. image limiting mag.: -7.91
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.68
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 12714 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 275.0067 to 290.7479 deg, Dec -7.2611 to +3.2758 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 275.0067 to 290.7479 deg, Dec -7.2611 to 3.2758 deg
Loaded 9411 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): 6787 out of 7189 total matches.
Matched with Tycho-2 7189 out of 12714 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits (aperture=6.3)
Read 16343 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 275.0005 to 290.7313 deg, Dec -7.2368 to +3.2867 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 275.0005 to 290.7313 deg, Dec -7.2368 to 3.2867 deg
Loaded 9368 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): 7209 out of 7793 total matches.
Matched with Tycho-2 7793 out of 16343 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
2.2 pix Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
2.7 pix fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
2.7 pix fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
Limiting magnitude estimates:
14.7 mag. Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
14.9 mag. Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
10.6 mag. fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
11.3 mag. fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
All-image limiting magnitude estimate: 10.6 (SNR ) 9.1 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.VqRTQDlevZ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.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-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits' -> 'wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1146, bad_region=3690, passed=12714
Got 12714 stars (including 8125 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat
util/solve_plate_with_UCAC5 got 12714 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 4798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 9726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4799 matched stars entering correct_measured_positions(), 9726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 4799 matched stars entering correct_measured_positions(), 9726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 4799 stars left (next iteration limit 5277)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits N_match=4799 sigma_overall_arcsec=0.557 sigma_q1_arcsec=0.593 sigma_q2_arcsec=0.577 sigma_q3_arcsec=0.491 sigma_q4_arcsec=0.524 n_q1=1529 n_q2=1228 n_q3=962 n_q4=1080 worst_quadrant_to_overall_ratio=1.063
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits -region wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.YpO0obEgax (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.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-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits' -> 'wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1609, bad_region=1765, passed=16343
Got 16343 stars (including 13061 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits.wcscat
util/solve_plate_with_UCAC5 got 16343 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 4844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 14972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 14972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 14972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 4845 stars left (next iteration limit 5328)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits N_match=4845 sigma_overall_arcsec=0.573 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.414 sigma_q3_arcsec=0.584 sigma_q4_arcsec=0.720 n_q1=1773 n_q2=552 n_q3=1577 n_q4=943 worst_quadrant_to_overall_ratio=1.256
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits -region wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.t9UETYjPjX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=87, bad_region=158, passed=1516
Got 1516 stars (including 1277 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits.wcscat
util/solve_plate_with_UCAC5 got 1516 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 414 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 1266 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1248 matched stars entering correct_measured_positions(), 1233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1248 matched stars entering correct_measured_positions(), 1399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 1266 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1249 matched stars entering correct_measured_positions(), 1397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Accuracy estimation diagnostic: 1249 matched stars entering correct_measured_positions(), 1397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Excluding outliers - 1249 stars left (next iteration limit 1372)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 1249 catalog matches do not cover the frame (743/2/403/101 per quadrant, need 78 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits N_match=1249 sigma_overall_arcsec=0.972 sigma_q1_arcsec=0.937 sigma_q2_arcsec=NaN sigma_q3_arcsec=1.070 sigma_q4_arcsec=0.807 n_q1=743 n_q2=2 n_q3=403 n_q4=101 worst_quadrant_to_overall_ratio=1.100
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits -region wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.vcNWYWj0av (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=90, bad_region=70, passed=1389
Got 1389 stars (including 1228 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits.wcscat
util/solve_plate_with_UCAC5 got 1389 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 414 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 1215 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1199 matched stars entering correct_measured_positions(), 1180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1199 matched stars entering correct_measured_positions(), 1312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 414 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 1215 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1198 matched stars entering correct_measured_positions(), 1313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Accuracy estimation diagnostic: 1198 matched stars entering correct_measured_positions(), 1312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Excluding outliers - 1198 stars left (next iteration limit 1318)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 1198 catalog matches do not cover the frame (459/8/675/56 per quadrant, need 74 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits N_match=1198 sigma_overall_arcsec=1.018 sigma_q1_arcsec=1.037 sigma_q2_arcsec=0.956 sigma_q3_arcsec=1.000 sigma_q4_arcsec=0.773 n_q1=459 n_q2=8 n_q3=675 n_q4=56 worst_quadrant_to_overall_ratio=1.019
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits -region wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits'
Saving the final (post-refit) wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits'
Saving the final (post-refit) wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits'
Saving the final (post-refit) wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits sigma_overall=0.557 worst_q_ratio=1.063
ref2=Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits sigma_overall=0.573 worst_q_ratio=1.256
new1=fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits sigma_overall=0.972 worst_q_ratio=1.100
new2=fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits sigma_overall=1.018 worst_q_ratio=1.019
reference average sigma_overall=0.565 worst_q_ratio=1.1595
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068_astrometric_residuals.png (4799 matched stars from wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046_astrometric_residuals.png (4845 matched stars from wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021_astrometric_residuals.png (1249 matched stars from wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.83 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022_astrometric_residuals.png (1198 matched stars from wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.87 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-50-48_20.00sec_0.00C_LIGHT_0021.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aql-03-Q2b1x1_235603_TTUQ2b1x1_2549458_Imc4pj8C/wcs_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022.fits'
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:17:54.70 -01:21:38.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:34.45 -03:52:20.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:38.71 -02:29:58.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:55.01 -03:44:52.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:54.61 -04:04:03.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:18:42.23 -01:39:39.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:34.59 +00:35:20.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:54.66 -04:02:54.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:17:56.67 -02:53:53.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:24.37 +00:29:35.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:34.59 +00:35:20.0: 10.59 +/- 0.00 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:38.71 -02:29:58.1: 10.48 +/- 0.00 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:54.66 -04:02:54.7: 10.87 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:55.01 -03:44:52.4: 10.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:54.61 -04:04:03.1: 10.98 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:34.45 -03:52:20.1: 10.69 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:17:54.70 -01:21:38.7: 10.65 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:17:56.67 -02:53:53.0: 10.21 +/- 0.00 detection
Forced photometry filter KEPT candidate at 19:16:34.59 +00:35:20.0: ref_mag=10.59 +/- 0.00 new_mean_mag=9.3903 delta=1.20 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:24.37 +00:29:35.6: 10.57 +/- 0.00 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:18:42.23 -01:39:39.8: 10.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.48 +/- 0.00
Forced photometry filter KEPT candidate at 19:16:38.71 -02:29:58.1: ref_mag=10.48 +/- 0.00 new_mean_mag=9.0885 delta=1.39 (need > 0.90)
Forced photometry reference-image weighted average: 10.44 +/- 0.00
Forced photometry reference-image weighted average: 10.98 +/- 0.01
Forced photometry reference-image weighted average: 10.87 +/- 0.01
Forced photometry reference-image weighted average: 10.69 +/- 0.01
Forced photometry filter KEPT candidate at 19:15:55.01 -03:44:52.4: ref_mag=10.44 +/- 0.00 new_mean_mag=9.2835 delta=1.16 (need > 0.90)
Forced photometry reference-image weighted average: 10.21 +/- 0.00
Forced photometry reference-image weighted average: 10.65 +/- 0.01
Forced photometry filter KEPT candidate at 19:15:54.61 -04:04:03.1: ref_mag=10.98 +/- 0.01 new_mean_mag=9.3739 delta=1.61 (need > 0.90)
Forced photometry filter KEPT candidate at 19:16:54.66 -04:02:54.7: ref_mag=10.87 +/- 0.01 new_mean_mag=9.3631 delta=1.50 (need > 0.90)
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Forced photometry filter KEPT candidate at 19:16:34.45 -03:52:20.1: ref_mag=10.69 +/- 0.01 new_mean_mag=9.4151 delta=1.28 (need > 0.90)
Forced photometry reference-image weighted average: 10.51 +/- 0.00
Forced photometry filter KEPT candidate at 19:17:56.67 -02:53:53.0: ref_mag=10.21 +/- 0.00 new_mean_mag=8.8075 delta=1.40 (need > 0.90)
Forced photometry filter KEPT candidate at 19:17:54.70 -01:21:38.7: ref_mag=10.65 +/- 0.01 new_mean_mag=9.2867 delta=1.36 (need > 0.90)
Forced photometry filter KEPT candidate at 19:16:24.37 +00:29:35.6: ref_mag=10.57 +/- 0.00 new_mean_mag=9.4137 delta=1.15 (need > 0.90)
Forced photometry filter KEPT candidate at 19:18:42.23 -01:39:39.8: ref_mag=10.51 +/- 0.00 new_mean_mag=9.1287 delta=1.38 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:17:27.15 -01:27:58.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:03.61 -02:38:13.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:51.79 -04:10:10.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:35.54 -01:57:03.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:17:27.15 -01:27:58.1: 10.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.42 +/- 0.00
Forced photometry filter KEPT candidate at 19:17:27.15 -01:27:58.1: ref_mag=10.42 +/- 0.00 new_mean_mag=9.3028 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:03.61 -02:38:13.4: 10.37 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.37 +/- 0.00
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:51.79 -04:10:10.0: 10.34 +/- 0.00 detection
Forced photometry filter KEPT candidate at 19:16:03.61 -02:38:13.4: ref_mag=10.37 +/- 0.00 new_mean_mag=9.0819 delta=1.29 (need > 0.90)
Forced photometry reference-image weighted average: 10.34 +/- 0.00
Forced photometry filter KEPT candidate at 19:15:51.79 -04:10:10.0: ref_mag=10.34 +/- 0.00 new_mean_mag=8.9162 delta=1.42 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:35.54 -01:57:03.1: 10.33 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.33 +/- 0.00
Forced photometry filter KEPT candidate at 19:16:35.54 -01:57:03.1: ref_mag=10.33 +/- 0.00 new_mean_mag=9.2936 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:26.62 -03:11:06.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:17:17.51 -02:32:12.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:26.62 -03:11:06.6: 10.31 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.31 +/- 0.00
Forced photometry filter KEPT candidate at 19:16:26.62 -03:11:06.6: ref_mag=10.31 +/- 0.00 new_mean_mag=9.2448 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:17:17.51 -02:32:12.5: 10.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.24 +/- 0.00
Forced photometry filter KEPT candidate at 19:17:17.51 -02:32:12.5: ref_mag=10.24 +/- 0.00 new_mean_mag=8.8698 delta=1.37 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:17:43.85 -01:41:50.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:17:43.85 -01:41:50.2: 10.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.22 +/- 0.00
Forced photometry filter KEPT candidate at 19:17:43.85 -01:41:50.2: ref_mag=10.22 +/- 0.00 new_mean_mag=9.1841 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:53.96 -03:14:16.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:53.96 -03:14:16.3: 10.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.20 +/- 0.00
Forced photometry filter KEPT candidate at 19:15:53.96 -03:14:16.3: ref_mag=10.20 +/- 0.00 new_mean_mag=9.2357 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:16:34.62 +00:45:57.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:16:34.62 +00:45:57.1: 10.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.14 +/- 0.00
Forced photometry filter KEPT candidate at 19:16:34.62 +00:45:57.1: ref_mag=10.14 +/- 0.00 new_mean_mag=9.0382 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:14:12.15 -03:45:34.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:14:12.15 -03:45:34.9: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.11 +/- 0.00
Forced photometry filter KEPT candidate at 19:14:12.15 -03:45:34.9: ref_mag=10.11 +/- 0.00 new_mean_mag=8.8138 delta=1.29 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:22.40 -03:39:08.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:22.40 -03:39:08.9: 10.08 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.08 +/- 0.00
Forced photometry filter KEPT candidate at 19:15:22.40 -03:39:08.9: ref_mag=10.08 +/- 0.00 new_mean_mag=9.1101 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:14:39.91 -03:52:16.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:14:39.91 -03:52:16.0: 10.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.04 +/- 0.00
Forced photometry filter KEPT candidate at 19:14:39.91 -03:52:16.0: ref_mag=10.04 +/- 0.00 new_mean_mag=8.7789 delta=1.26 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:17:07.05 -02:27:44.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:17:07.05 -02:27:44.1: 10.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.03 +/- 0.00
Forced photometry filter KEPT candidate at 19:17:07.05 -02:27:44.1: ref_mag=10.03 +/- 0.00 new_mean_mag=8.7649 delta=1.27 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:24.68 -04:04:46.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:17:13.91 -02:15:12.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:12:02.69 -02:31:53.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:24.68 -04:04:46.3: 10.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.02 +/- 0.00
Forced photometry filter KEPT candidate at 19:15:24.68 -04:04:46.3: ref_mag=10.02 +/- 0.00 new_mean_mag=8.7236 delta=1.30 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:17:13.91 -02:15:12.0: 9.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.99 +/- 0.00
Forced photometry filter KEPT candidate at 19:17:13.91 -02:15:12.0: ref_mag=9.99 +/- 0.00 new_mean_mag=8.8393 delta=1.15 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:12:02.69 -02:31:53.3: 9.89 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.89 +/- 0.00
Forced photometry filter KEPT candidate at 19:12:02.69 -02:31:53.3: ref_mag=9.89 +/- 0.00 new_mean_mag=8.7711 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:11:49.85 -02:22:48.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:12:57.58 -03:12:27.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:14:57.26 -03:18:01.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:18:43.41 -03:08:12.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:11:49.85 -02:22:48.4: 9.85 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.85 +/- 0.00
Forced photometry filter KEPT candidate at 19:11:49.85 -02:22:48.4: ref_mag=9.85 +/- 0.00 new_mean_mag=8.7862 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:12:57.58 -03:12:27.9: 9.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.84 +/- 0.00
Forced photometry filter KEPT candidate at 19:12:57.58 -03:12:27.9: ref_mag=9.84 +/- 0.00 new_mean_mag=8.8011 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:18:41.66 -03:05:51.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:14:57.26 -03:18:01.3: 9.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.82 +/- 0.00
Forced photometry filter KEPT candidate at 19:14:57.26 -03:18:01.3: ref_mag=9.82 +/- 0.00 new_mean_mag=8.9143 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:18:43.41 -03:08:12.4: 9.74 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.74 +/- 0.00
Forced photometry filter KEPT candidate at 19:18:43.41 -03:08:12.4: ref_mag=9.74 +/- 0.00 new_mean_mag=8.6913 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:18:41.66 -03:05:51.7: 9.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.73 +/- 0.00
Forced photometry filter KEPT candidate at 19:18:41.66 -03:05:51.7: ref_mag=9.73 +/- 0.00 new_mean_mag=8.5695 delta=1.16 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:15:31.97 -04:10:03.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:15:31.97 -04:10:03.8: 9.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.58 +/- 0.00
Forced photometry filter KEPT candidate at 19:15:31.97 -04:10:03.8: ref_mag=9.58 +/- 0.00 new_mean_mag=8.4039 delta=1.18 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:18:37.70 +00:28:45.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:18:41.24 -01:53:13.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:18:37.70 +00:28:45.9: 9.54 +/- 0.00 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:17:46.09 +00:36:37.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 9.54 +/- 0.00
Forced photometry filter KEPT candidate at 19:18:37.70 +00:28:45.9: ref_mag=9.54 +/- 0.00 new_mean_mag=8.3848 delta=1.16 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-08_01-31-19_20.00sec_4.90C_LIGHT_0068.fits at 19:18:20.51 +00:44:39.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:18:41.24 -01:53:13.4: 9.47 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.47 +/- 0.00
Forced photometry filter KEPT candidate at 19:18:41.24 -01:53:13.4: ref_mag=9.47 +/- 0.00 new_mean_mag=8.4644 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:17:46.09 +00:36:37.6: 9.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.43 +/- 0.00
Forced photometry filter KEPT candidate at 19:17:46.09 +00:36:37.6: ref_mag=9.43 +/- 0.00 new_mean_mag=8.4563 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-07-13_01-31-23_20.00sec_4.90C_LIGHT_0046.fits at 19:18:20.51 +00:44:39.3: 9.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.15 +/- 0.00
Forced photometry filter KEPT candidate at 19:18:20.51 +00:44:39.3: ref_mag=9.15 +/- 0.00 new_mean_mag=8.1694 delta=0.98 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out20206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21064.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 36s
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 20473_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20473_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:17:56.67 -02:53:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.93, MAG_FAINT_SEARCH_LIMIT=9.91)GAIADR2_OUTPUT=# 0.439 4213063820168728064 289.48603122707 -02.89813351534 9.7993 8.9694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21064_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 21064_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20947_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20947_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20783_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20783_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20738_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20738_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:17:54.70 -01:21:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.29, MAG_FAINT_SEARCH_LIMIT=10.27)GAIADR2_OUTPUT=# 0.684 4262976494120827008 289.47808557357 -01.36083698659 10.0362 9.0722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20704_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20704_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20688_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20688_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20645_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20645_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20622_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20622_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:16:38.71 -02:29:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.12, MAG_FAINT_SEARCH_LIMIT=10.10)GAIADR2_OUTPUT=# 1.126 4261161921969691904 289.16159686152 -02.49940277724 9.8713 8.8708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20595_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20595_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:15:55.01 -03:44:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.27, MAG_FAINT_SEARCH_LIMIT=10.25)GAIADR2_OUTPUT=# 0.812 4212864499325955968 288.97939598498 -03.74801451052 10.0467 9.2713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20581_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20581_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:17:27.15 -01:27:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.29, MAG_FAINT_SEARCH_LIMIT=10.27)GAIADR2_OUTPUT=# 0.388 4262973844104790272 289.36318675247 -01.46622726912 10.0208 9.2035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20553_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20553_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20539_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20539_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20536_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20536_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:16:35.54 -01:57:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.28, MAG_FAINT_SEARCH_LIMIT=10.26)GAIADR2_OUTPUT=# 0.281 4261232015838665856 289.14803473780 -01.95079995380 9.9161 9.1114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20531_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20531_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:16:26.62 -03:11:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.23, MAG_FAINT_SEARCH_LIMIT=10.21)GAIADR2_OUTPUT=# 1.433 4212958541932773888 289.11055566869 -03.18499792382 10.0643 9.5356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20498_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20498_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20484_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20484_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:17:43.85 -01:41:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.16, MAG_FAINT_SEARCH_LIMIT=10.14)GAIADR2_OUTPUT=# 0.616 4262756042031866496 289.43255517767 -01.69720119761 10.0478 9.6835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20467_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20467_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:15:53.96 -03:14:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.21, MAG_FAINT_SEARCH_LIMIT=10.19)GAIADR2_OUTPUT=# 0.389 4212968334458267904 288.97491821951 -03.23779427758 9.6995 8.8046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20445_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20445_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:16:34.62 +00:45:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.05, MAG_FAINT_SEARCH_LIMIT=10.03)GAIADR2_OUTPUT=# 2.969 4264636241290884736 289.14504724775 +00.76607291089 9.4857 8.4654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20432_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20432_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:14:12.15 -03:45:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.95, MAG_FAINT_SEARCH_LIMIT=9.93)GAIADR2_OUTPUT=# 0.177 4212911159852273408 288.55061133379 -03.75974159227 9.9116 9.5124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20427_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20427_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:15:22.40 -03:39:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.10, MAG_FAINT_SEARCH_LIMIT=10.08)GAIADR2_OUTPUT=# 0.252 4212916000259504512 288.84326685762 -03.65244982030 9.7979 9.2569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20417_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20417_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:14:39.91 -03:52:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.88, MAG_FAINT_SEARCH_LIMIT=9.86)GAIADR2_OUTPUT=# 0.612 4212859547209369856 288.66619394460 -03.87097189724 9.7783 9.2184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20413_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20413_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:17:07.05 -02:27:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.90, MAG_FAINT_SEARCH_LIMIT=9.88)GAIADR2_OUTPUT=# 0.864 4261152129444191232 289.27914623540 -02.46217631213 9.7767 9.2149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20407_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20407_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20392_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20392_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:17:13.91 -02:15:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.96, MAG_FAINT_SEARCH_LIMIT=9.94)GAIADR2_OUTPUT=# 0.386 4261175494066494592 289.30805583018 -02.25337830933 9.5232 8.6746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20358_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20358_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:12:02.69 -02:31:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.93, MAG_FAINT_SEARCH_LIMIT=9.91)GAIADR2_OUTPUT=# 0.774 4261288709388666112 288.01099951615 -02.53152394080 9.7022 9.2233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20350_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20350_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:11:49.85 -02:22:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.88, MAG_FAINT_SEARCH_LIMIT=9.86)GAIADR2_OUTPUT=# 0.548 4261299532731630080 287.95768514878 -02.37996061523 9.6020 9.1166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20347_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20347_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:12:57.58 -03:12:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.91, MAG_FAINT_SEARCH_LIMIT=9.89)GAIADR2_OUTPUT=# 0.949 4260996097560829568 288.23965425141 -03.20777845821 9.5959 9.0967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20335_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20335_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:14:57.26 -03:18:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.96, MAG_FAINT_SEARCH_LIMIT=9.94)GAIADR2_OUTPUT=# 0.311 4212963970771644672 288.73854554465 -03.30043877503 9.4427 8.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20319_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20319_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:18:43.41 -03:08:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.78, MAG_FAINT_SEARCH_LIMIT=9.76)GAIADR2_OUTPUT=# 1.395 4213008221804972928 289.68050258719 -03.13666853802 9.5662 9.1602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20312_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20312_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:18:41.66 -03:05:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.69, MAG_FAINT_SEARCH_LIMIT=9.67)GAIADR2_OUTPUT=# 1.715 4213010012816631552 289.67405495242 -03.09762308420 8.6624 7.4195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20276_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
Preparing report for the candidate 20276_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
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Considering the candidate 20269_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20269_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:18:37.70 +00:28:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.41, MAG_FAINT_SEARCH_LIMIT=9.39)GAIADR2_OUTPUT=# 1.255 4264379230443673088 289.65726912347 +00.47971158204 9.1685 8.4047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20254_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20254_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:18:41.24 -01:53:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.55, MAG_FAINT_SEARCH_LIMIT=9.53)GAIADR2_OUTPUT=# 1.577 4262690513697799552 289.67226513694 -01.88698028463 9.1066 8.3437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20249_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20249_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:17:46.09 +00:36:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.46, MAG_FAINT_SEARCH_LIMIT=9.44)GAIADR2_OUTPUT=# 1.719 4264430392096973568 289.44195039137 +00.61091300418 9.3715 9.1980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20206_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20206_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
**** FOUND 19:18:20.51 +00:44:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.20, MAG_FAINT_SEARCH_LIMIT=9.18)GAIADR2_OUTPUT=# 4.098 4264457123974680448 289.58635522145 +00.74495086943 7.7369 6.3868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20185_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022
The candidate 20185_fd_Aql-03-Q2b1x1_2026-09-08_23-51-35_20.00sec_-0.00C_LIGHT_0022 did not pass the final checks
