This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 10.04 18:17:54.90 -12:00:42.6
18.43361 1.83260 galactic Ser Second-epoch detections are separated by 0.8" and 9.1 pix
The object was found in VSX 2" ASASSN-V J181755.04-120042.9
Type: L
# Max. Min./Amp. JD0 Period
11.600 V 12.130 V
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:17:54.90 -12:00:42.6: 10.95 +/- 0.01 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:17:54.90 -12:00:42.6: 11.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.97 +/- 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!
TCP 2026 05 26.2021* 18 17 54.90 -12 00 42.6 10.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181755.04-120042.9,2461186.7021,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181755.04-120042.9 20260526.2021 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.24 18:22:00.74 -06:57:49.0
23.36885 3.31534 galactic Sct Second-epoch detections are separated by 1.3" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.51 Nemausa 3 -0 3 11.2 -0 0
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:22:00.74 -06:57:49.0: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:22:00.74 -06:57:49.0: 15.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461186.7021,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.2021 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 9.51 18:18:18.28 -12:10:56.9
18.32829 1.66795 galactic Ser Second-epoch detections are separated by 0.1" and 9.2 pix
The object was found in VSX 1" ASAS J181818-1211.0
Type: SRB
# Max. Min./Amp. JD0 Period
10.850 V 11.530 V 2454302.00000 66.700000000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:18:18.28 -12:10:56.9: 10.51 +/- 0.01 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:18:18.28 -12:10:56.9: 10.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.46 +/- 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!
TCP 2026 05 26.2021* 18 18 18.28 -12 10 56.9 9.5 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J181818-1211.0,2461186.7021,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J181818-1211.0 20260526.2021 9.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.51 18:12:02.53 -13:02:57.6
16.83769 2.59900 galactic Ser Second-epoch detections are separated by 1.9" and 9.5 pix
The object was found in VSX 1" ASASSN-V J181202.61-130257.9
Type: L
# Max. Min./Amp. JD0 Period
13.520 V 13.800 V
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:12:02.53 -13:02:57.6: 12.60 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:12:02.53 -13:02:57.6: 12.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 12 02.53 -13 02 57.6 11.5 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181202.61-130257.9,2461186.7021,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181202.61-130257.9 20260526.2021 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.87 18:09:46.63 -14:33:46.6
15.24459 2.35372 galactic Ser Second-epoch detections are separated by 2.7" and 9.1 pix
The object was found in VSX 1" ASASSN-V J180946.65-143347.3
Type: SRS
# Max. Min./Amp. JD0 Period
13.690 V 13.790 V 2458237.93500 19.978000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:09:46.63 -14:33:46.6: 12.87 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:09:46.63 -14:33:46.6: 12.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 09 46.63 -14 33 46.6 11.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180946.65-143347.3,2461186.7021,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180946.65-143347.3 20260526.2021 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.91 18:11:23.07 -14:53:14.5
15.14729 1.85691 galactic Ser Second-epoch detections are separated by 2.9" and 9.6 pix
The object was found in VSX 5" Gaia DR3 4146098442474057216
Type: L
# Max. Min./Amp. JD0 Period
18.910 G 19.580 G
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:11:23.07 -14:53:14.5: 12.91 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:11:23.07 -14:53:14.5: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 11 23.07 -14 53 14.5 11.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146098442474057216,2461186.7021,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4146098442474057216 20260526.2021 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.12 17:39:47.55 -07:25:34.0
17.86033 12.26779 galactic Oph Second-epoch detections are separated by 0.7" and 9.2 pix
The object was found in VSX 1" ASASSN-V J173947.49-072533.1
Type: SR
# Max. Min./Amp. JD0 Period
15.230 g Y 0.470 g 2459384.81800 304.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:39:47.55 -07:25:34.0: 13.15 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:39:47.55 -07:25:34.0: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173947.49-072533.1,2461186.7021,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173947.49-072533.1 20260526.2021 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.60 17:31:33.03 -09:48:28.5
14.69952 12.81861 galactic Oph Second-epoch detections are separated by 1.6" and 9.6 pix
The object was found in VSX 2" ASAS J173133-0948.5
Type: SR|EC|ESD
# Max. Min./Amp. JD0 Period
9.116 Ic Y 0.150 Ic 2452424.40000 27.303000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:31:33.03 -09:48:28.5: 12.70 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:31:33.03 -09:48:28.5: 12.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173133-0948.5,2461186.7021,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173133-0948.5 20260526.2021 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.07 18:08:14.74 -14:52:56.0
14.78574 2.52371 galactic Ser Second-epoch detections are separated by 2.7" and 9.1 pix
The object was found in VSX 1" ASASSN-V J180814.74-145256.6
Type: SR
# Max. Min./Amp. JD0 Period
15.190 g Y 0.300 g 2459484.59000 587.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:08:14.74 -14:52:56.0: 13.29 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:08:14.74 -14:52:56.0: 13.45 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 08 14.74 -14 52 56.0 12.1 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180814.74-145256.6,2461186.7021,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180814.74-145256.6 20260526.2021 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.29 17:37:21.35 -07:02:36.5
17.89072 12.98244 galactic Oph Second-epoch detections are separated by 1.9" and 9.1 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 J264.3386-07.0431 | 17:37:21.27 -07:02:35.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.606+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:37:21.35 -07:02:36.5: 13.42 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:37:21.35 -07:02:36.5: 13.26 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J264.3386-07.0431,2461186.7021,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J264.3386-07.0431 20260526.2021 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.00 17:41:46.67 -06:27:40.7
18.96782 12.31937 galactic Oph Second-epoch detections are separated by 1.0" and 9.4 pix
The object was found in VSX 2" NSV 23458
Type: SR:
# Max. Min./Amp. JD0 Period
13.200 V < 14.500 V 165.000000000000 M8III
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:41:46.67 -06:27:40.7: 12.61 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:41:46.67 -06:27:40.7: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 23458,2461186.7021,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 23458 20260526.2021 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.23 18:19:01.00 -11:18:23.0
19.18318 1.92830 galactic Ser Second-epoch detections are separated by 1.2" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.7730 Sergerasimov 188 -69 200 16.5 -0 -0
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:19:01.00 -11:18:23.0: 13.44 +/- 0.06 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:19:01.00 -11:18:23.0: 13.51 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 19 01.00 -11 18 23.0 12.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461186.7021,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.2021 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.82 18:21:09.30 -10:21:48.2
20.26293 1.90921 galactic Ser Second-epoch detections are separated by 1.1" and 9.4 pix
The object was found in VSX 2" ASASSN-V J182109.41-102146.9
Type: L
# Max. Min./Amp. JD0 Period
13.800 V 14.220 V
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:21:09.30 -10:21:48.2: 12.65 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:21:09.30 -10:21:48.2: 13.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 21 09.30 -10 21 48.2 11.8 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J182109.41-102146.9,2461186.7021,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J182109.41-102146.9 20260526.2021 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.91 18:13:52.99 -14:40:55.3
15.61721 1.42526 galactic Ser Second-epoch detections are separated by 1.2" and 9.0 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 J273.4711-14.6825 | 18:13:53.05 -14:40:57.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.572+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:13:52.99 -14:40:55.3: 12.92 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:13:52.99 -14:40:55.3: 13.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 13 52.99 -14 40 55.3 11.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.4711-14.6825,2461186.7021,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.4711-14.6825 20260526.2021 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.24 18:17:02.91 -12:57:33.1
17.49872 1.56998 galactic Ser Second-epoch detections are separated by 4.7" and 9.6 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 J274.2623-12.9594 | 18:17:02.91 -12:57:33.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.306+/-0.037 (Very red! L if it's a dwarf)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:17:02.91 -12:57:33.1: 13.42 +/- 0.06 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:17:02.91 -12:57:33.1: 13.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 17 02.91 -12 57 33.1 12.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.2623-12.9594,2461186.7021,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.2623-12.9594 20260526.2021 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.38 18:18:01.22 -11:29:13.5
18.90840 2.05813 galactic Ser Second-epoch detections are separated by 1.5" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4153910227718312704 | 18:18:01.26 -11:29:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.640+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:18:01.22 -11:29:13.5: 13.40 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:18:01.22 -11:29:13.5: 13.54 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 18 01.22 -11 29 13.5 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4153910227718312704,2461186.7021,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4153910227718312704 20260526.2021 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.54 18:11:30.94 -14:54:25.2
15.14530 1.81968 galactic Ser Second-epoch detections are separated by 1.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4146095345744484864 | 18:11:31.02 -14:54:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.510+/-0.037 (Very red! L if it's a dwarf)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:11:30.94 -14:54:25.2: 12.65 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:11:30.94 -14:54:25.2: 12.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 11 30.94 -14 54 25.2 11.5 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146095345744484864,2461186.7021,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4146095345744484864 20260526.2021 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 10.97 18:23:28.49 -08:54:07.4
21.82275 2.08910 galactic Sct Second-epoch detections are separated by 0.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.216 Kleopatra 2 -1 2 11.9 -0 0
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:23:28.49 -08:54:07.4: 12.30 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:23:28.49 -08:54:07.4: 12.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461186.7021,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.2021 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.15 18:24:58.13 -10:46:08.8
20.34369 0.89108 galactic Sct Second-epoch detections are separated by 1.2" and 9.4 pix
The object was found in VSX 1" Gaia DR3 4154231667392734976
Type: L
# Max. Min./Amp. JD0 Period
11.540 G 11.680 G M
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:24:58.13 -10:46:08.8: 13.27 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:24:58.13 -10:46:08.8: 13.60 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.05
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 4154231667392734976,2461186.7021,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4154231667392734976 20260526.2021 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.90 18:14:18.74 -14:11:16.8
16.10102 1.57000 galactic Ser Second-epoch detections are separated by 2.7" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J273.5782-14.1880 | 18:14:18.78 -14:11:17.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.388+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:14:18.74 -14:11:16.8: 12.91 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:14:18.74 -14:11:16.8: 12.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 14 18.74 -14 11 16.8 11.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.5782-14.1880,2461186.7021,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.5782-14.1880 20260526.2021 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.25 18:15:03.15 -13:57:36.1
16.38711 1.52100 galactic Ser Second-epoch detections are separated by 1.9" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J273.7633-13.9602 | 18:15:03.18 -13:57:36.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.513+/-0.040 (Very red! L if it's a dwarf)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:15:03.15 -13:57:36.1: 12.27 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:15:03.15 -13:57:36.1: 12.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 15 03.15 -13 57 36.1 11.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.7633-13.9602,2461186.7021,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.7633-13.9602 20260526.2021 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 10.71 18:13:23.58 -15:02:58.7
15.23762 1.35343 galactic Ser Second-epoch detections are separated by 1.9" and 8.9 pix
The object was found in VSX 3" ASAS J181324-1503.0
Type: MISC
# Max. Min./Amp. JD0 Period
8.793 Ic Y 0.251 Ic 2452890.50000 172.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:13:23.58 -15:02:58.7: 11.85 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:13:23.58 -15:02:58.7: 11.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.83 +/- 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!
TCP 2026 05 26.2021* 18 13 23.58 -15 02 58.7 10.7 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J181324-1503.0,2461186.7021,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J181324-1503.0 20260526.2021 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.29 17:40:10.30 -07:30:54.7
17.82931 12.14189 galactic Oph Second-epoch detections are separated by 1.6" and 9.1 pix
The object was found in VSX 1" ASASSN-V J174010.34-073054.0
Type: SRS
# Max. Min./Amp. JD0 Period
14.990 g Y 0.350 g 2458587.89500 26.157000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:40:10.30 -07:30:54.7: 13.26 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:40:10.30 -07:30:54.7: 13.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174010.34-073054.0,2461186.7021,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174010.34-073054.0 20260526.2021 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.31 18:09:53.77 -14:36:22.6
15.22049 2.30761 galactic Ser Second-epoch detections are separated by 2.8" and 9.3 pix
The object was found in VSX 2" ASASSN-V J180953.87-143623.0
Type: SR
# Max. Min./Amp. JD0 Period
13.780 g Y 0.150 g 2459299.65500 561.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:09:53.77 -14:36:22.6: 12.24 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:09:53.77 -14:36:22.6: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 09 53.77 -14 36 22.6 11.3 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180953.87-143623.0,2461186.7021,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180953.87-143623.0 20260526.2021 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.47 17:32:25.58 -07:29:59.5
16.85318 13.80949 galactic Oph Second-epoch detections are separated by 0.8" and 9.3 pix
The object was found in VSX 2" ASAS J173225-0730.0
Type: MISC
# Max. Min./Amp. JD0 Period
9.005 Ic Y 0.236 Ic 2452528.00000 77.560000000000
The object was found in astcheck.19706 1999 TU11 422 -222 477 16.7 0 0
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:32:25.58 -07:29:59.5: 12.54 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:32:25.58 -07:29:59.5: 12.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173225-0730.0,2461186.7021,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173225-0730.0 20260526.2021 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.28 18:26:11.51 -07:43:43.7
23.17492 2.04180 galactic Sct Second-epoch detections are separated by 1.6" and 9.5 pix
The object was found in ASASSN-V 4" ASASSN-V J182611.56-074347.3
Type: SR
MeanMag 15.01 m Amp. 0.68 m Period 600.4792316 d
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:26:11.51 -07:43:43.7: 13.38 +/- 0.06 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:26:11.51 -07:43:43.7: 13.52 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.05
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
VARIABLE_NAME,2461186.7021,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.2021 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.95 18:12:43.36 -14:53:11.5
15.30328 1.57367 galactic Ser Second-epoch detections are separated by 1.3" and 8.9 pix
The object was found in VSX 1" ASASSN-V J181243.37-145312.8
Type: SRS
# Max. Min./Amp. JD0 Period
14.860 g Y 0.240 g 2458777.50900 26.762000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:12:43.36 -14:53:11.5: 13.05 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:12:43.36 -14:53:11.5: 13.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 12 43.36 -14 53 11.5 11.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181243.37-145312.8,2461186.7021,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181243.37-145312.8 20260526.2021 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 10.65 18:13:02.61 -12:16:36.0
17.63392 2.75414 galactic Ser Second-epoch detections are separated by 0.8" and 9.2 pix
The object was found in VSX 1" ASASSN-V J181302.67-121635.9
Type: L
# Max. Min./Amp. JD0 Period
12.310 V 12.590 V
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:13:02.61 -12:16:36.0: 11.73 +/- 0.01 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:13:02.61 -12:16:36.0: 11.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 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!
TCP 2026 05 26.2021* 18 13 02.61 -12 16 36.0 10.7 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181302.67-121635.9,2461186.7021,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181302.67-121635.9 20260526.2021 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.39 18:19:19.44 -12:47:57.6
17.90214 1.15714 galactic Ser Second-epoch detections are separated by 2.3" and 8.9 pix
The object was found in VSX15" Gaia DR3 4152737186262204160
Type: L
# Max. Min./Amp. JD0 Period
18.710 G 19.230 G
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:19:19.44 -12:47:57.6: 14.01 +/- 0.10 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:19:19.44 -12:47:57.6: 13.96 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 19 19.44 -12 47 57.6 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4152737186262204160,2461186.7021,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4152737186262204160 20260526.2021 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.05 18:26:36.94 -07:31:49.8
23.39946 2.04107 galactic Sct Second-epoch detections are separated by 1.4" and 9.4 pix
The object was found in VSX 3" GDS_J1826371-073148
Type: SR
# Max. Min./Amp. JD0 Period
13.320 r Y 0.330 r 2458607.52050 36.900767600000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:26:36.94 -07:31:49.8: 13.02 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:26:36.94 -07:31:49.8: 13.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1826371-073148,2461186.7021,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1826371-073148 20260526.2021 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.28 18:24:09.52 -10:37:37.4
20.37624 1.13342 galactic Sct Second-epoch detections are separated by 0.9" and 9.3 pix
The object was found in VSX 3" V0497 Sct
Type: SRB
# Max. Min./Amp. JD0 Period
12.900 V 14.100 V 2454577.00000 188.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:24:09.52 -10:37:37.4: 12.16 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:24:09.52 -10:37:37.4: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0497 Sct,2461186.7021,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0497 Sct 20260526.2021 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.77 18:12:31.56 -14:21:36.0
15.74279 1.86779 galactic Ser Second-epoch detections are separated by 1.5" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J273.1317-14.3600 | 18:12:31.61 -14:21:36.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.669+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:12:31.56 -14:21:36.0: 12.80 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:12:31.56 -14:21:36.0: 12.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 12 31.56 -14 21 36.0 11.8 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.1317-14.3600,2461186.7021,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.1317-14.3600 20260526.2021 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.71 18:18:49.64 -12:30:44.7
18.09783 1.39947 galactic Ser Second-epoch detections are separated by 2.4" and 9.5 pix
The object was found in VSX 3" ASASSN-V J181849.79-123046.7
Type: SR
# Max. Min./Amp. JD0 Period
13.780 V 13.940 V 2457879.97300 61.060000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:18:49.64 -12:30:44.7: 12.99 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:18:49.64 -12:30:44.7: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 18 49.64 -12 30 44.7 11.7 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181849.79-123046.7,2461186.7021,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181849.79-123046.7 20260526.2021 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 11.11 18:19:51.46 -12:04:09.1
18.60752 1.38686 galactic Ser Second-epoch detections are separated by 0.5" and 9.2 pix
The object was found in VSX 1" ASASSN-V J181951.54-120409.5
Type: SR
# Max. Min./Amp. JD0 Period
13.040 V 13.250 V 2458008.54000 39.770000000000
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:19:51.46 -12:04:09.1: 12.11 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:19:51.46 -12:04:09.1: 12.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.15 +/- 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!
TCP 2026 05 26.2021* 18 19 51.46 -12 04 09.1 11.1 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181951.54-120409.5,2461186.7021,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181951.54-120409.5 20260526.2021 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.00 18:08:46.70 -13:46:00.8
15.82568 2.94987 galactic Ser Second-epoch detections are separated by 0.5" and 9.1 pix
The object was found in VSX 1" ASASSN-V J180846.76-134601.5
Type: L:
# Max. Min./Amp. JD0 Period
13.890 V 14.170 V
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:08:46.70 -13:46:00.8: 12.99 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:08:46.70 -13:46:00.8: 12.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2021* 18 08 46.70 -13 46 00.8 12.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180846.76-134601.5,2461186.7021,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180846.76-134601.5 20260526.2021 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.05 18:24:12.30 -11:26:53.1
19.65582 0.73927 galactic Sct Second-epoch detections are separated by 0.6" and 9.3 pix
The object was found in VSX 1" GDS_J1824123-112652
Type: VAR
# Max. Min./Amp. JD0 Period
12.430 r Y 0.380 r
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:24:12.30 -11:26:53.1: 13.00 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:24:12.30 -11:26:53.1: 13.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1824123-112652,2461186.7021,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1824123-112652 20260526.2021 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2021 2461186.7021 12.23 18:24:52.68 -08:36:53.9
22.23877 1.91661 galactic Sct Second-epoch detections are separated by 2.5" and 9.7 pix
The object was found in VSX 0" NSVS 13825682
Type: L
# Max. Min./Amp. JD0 Period
12.400 R1 12.800 R1
The object was not found in astcheck.
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:24:52.68 -08:36:53.9: 13.18 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:24:52.68 -08:36:53.9: 13.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13825682,2461186.7021,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13825682 20260526.2021 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461120.93253516 21.03.2026 10:22:41.038 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
First image: 2461120.93253516 21.03.2026 10:22:41.038 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
Last image: 2461186.70242437 26.05.2026 04:51:19.466 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.11
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6618
Objects passed selection criteria: 6598
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 5258.75
Average stars matched: 5141.25 (97.7656 %)
Memory usage VmPeak: 114464 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 23:55:30 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461120.93253516 21.03.2026 10:22:41.038 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
First image: 2461120.93253516 21.03.2026 10:22:41.038 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
Last image: 2461186.70242437 26.05.2026 04:51:19.466 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 152
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.83
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: 15 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 72135
Objects passed selection criteria: 71977
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 49561.8
Average stars matched: 47245.8 (95.327 %)
Memory usage VmPeak: 178744 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 23:58:23 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
SExtractor catalog cache: saved Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat to cache
SExtractor catalog cache: saved Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.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/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461186.70187311
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_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits exists and is non-empty
Saving wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits to local_wcs_cache/
'wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits' -> 'local_wcs_cache/wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits'
wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
Saving wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits to local_wcs_cache/
'wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'local_wcs_cache/wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits exists and is non-empty
Saving wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits to local_wcs_cache/
'wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits' -> 'local_wcs_cache/wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits'
wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits exists and is non-empty
Saving wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits to local_wcs_cache/
'wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits' -> 'local_wcs_cache/wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits (1st reference image)
verification OK: wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
Image size: 937.8'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:00:09.727 -10:00:51.37 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/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_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits (1st new image)
verification OK: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
Image size: 942.1'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:00:01.471 -10:00:01.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:00:09.727 -10:00:51.37
Second-epoch image center 18:00:01.471 -10:00:01.34
Angular distance between the image centers 0.0366 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits (2nd new image)
verification OK: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Image size: 942.1'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 17:59:58.751 -10:00:39.19 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:00:09.727 -10:00:51.37
Second-epoch image center 17:59:58.751 -10:00:39.19
Angular distance between the image centers 0.0452 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 18:00:01.471 -10:00:01.34
Second-epoch second image center 17:59:58.751 -10:00:39.19
Angular distance between the image centers 0.01533 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits &> /tmp/tmp.hN7tmsML6G
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.kFptF8Ulvw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits &> /tmp/tmp.1YBjur1eiK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits &> /tmp/tmp.1BP0VmqQyb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.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_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits and wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits and wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
Found non-empty wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits and wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
The reference image (wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits) and catalog (wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat) found
'wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat' -> 'wcsmag.cat'
Read 10906 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 261.9133 to 278.0919 deg, Dec -15.2882 to -4.7064 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 261.9133 to 278.0919 deg, Dec -15.2882 to -4.7064 deg
Loaded 6344 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): 4993 out of 5278 total matches.
Matched with Tycho-2 5278 out of 10906 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.875000
a=0.000000 b=1.000000 c=22.875000
From vast_summary.log: estimated ref. image limiting mag.: -8.11
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.77
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.77
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 10906 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 261.9133 to 278.0919 deg, Dec -15.2882 to -4.7064 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 261.9133 to 278.0919 deg, Dec -15.2882 to -4.7064 deg
Loaded 6344 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): 4993 out of 5278 total matches.
Matched with Tycho-2 5278 out of 10906 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits:
Forced-photometry filter: calibrated wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits -> calib.txt_param_ref_wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits (aperture=6.6)
Read 7040 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 261.5744 to 278.1766 deg, Dec -15.6655 to -4.2025 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 261.5744 to 278.1766 deg, Dec -15.6655 to -4.2025 deg
Loaded 7311 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): 4311 out of 4538 total matches.
Matched with Tycho-2 4538 out of 7040 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: calibrated wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.6 pix Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
2.2 pix Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
4.2 pix fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
4.2 pix fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
2.6 pix wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
2.2 pix wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Limiting magnitude estimates:
14.8 mag. Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
14.5 mag. Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
12.2 mag. fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
12.2 mag. fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 10.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hN7tmsML6G (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits' -> 'wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
WCS_IMAGE_NAME=wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
WCS-calibrated image found: wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
Checking if the catalog wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat corresponding to the image wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits alredy exist and is non-empty...
Catalog wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat corresponding to the image wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
WCS catalog name: wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=810, passed=10906
Got 10906 stars (including 10078 good ones) from the SExtractor catalog wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
util/solve_plate_with_UCAC5 got 10906 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 10318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 10316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 10316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits N_match=921 sigma_overall_arcsec=0.622 sigma_q1_arcsec=0.545 sigma_q2_arcsec=0.793 sigma_q3_arcsec=0.544 sigma_q4_arcsec=0.581 n_q1=237 n_q2=412 n_q3=131 n_q4=141 worst_quadrant_to_overall_ratio=1.275
The image catalog is written to wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits -region wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kFptF8Ulvw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat corresponding to the image wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat corresponding to the image wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=587, passed=7040
Got 7040 stars (including 6440 good ones) from the SExtractor catalog wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
util/solve_plate_with_UCAC5 got 7040 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.4'
Seting catalog search parameters based on the expected field of view 942.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013089 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010471 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 6677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 6674 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 6674 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=922 sigma_overall_arcsec=0.387 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.412 sigma_q4_arcsec=0.447 n_q1=232 n_q2=399 n_q3=156 n_q4=135 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1YBjur1eiK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
WCS_IMAGE_NAME=wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
WCS-calibrated image found: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
Checking if the catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat corresponding to the image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat corresponding to the image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
WCS catalog name: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=84, passed=1632
Got 1632 stars (including 1546 good ones) from the SExtractor catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat
util/solve_plate_with_UCAC5 got 1632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 1541 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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 1538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 1538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits N_match=909 sigma_overall_arcsec=0.565 sigma_q1_arcsec=0.666 sigma_q2_arcsec=0.590 sigma_q3_arcsec=0.395 sigma_q4_arcsec=0.485 n_q1=224 n_q2=403 n_q3=143 n_q4=139 worst_quadrant_to_overall_ratio=1.178
The image catalog is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits -region wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1BP0VmqQyb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
WCS_IMAGE_NAME=wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
WCS-calibrated image found: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Checking if the catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat corresponding to the image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat corresponding to the image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
WCS catalog name: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=83, passed=1687
Got 1687 stars (including 1601 good ones) from the SExtractor catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat
util/solve_plate_with_UCAC5 got 1687 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 1598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 1598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 1598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 909 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits N_match=909 sigma_overall_arcsec=0.577 sigma_q1_arcsec=0.703 sigma_q2_arcsec=0.653 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.506 n_q1=214 n_q2=414 n_q3=142 n_q4=139 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits -region wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits sigma_overall=0.622 worst_q_ratio=1.275
ref2=Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits sigma_overall=0.387 worst_q_ratio=1.155
new1=fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits sigma_overall=0.565 worst_q_ratio=1.178
new2=fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits sigma_overall=0.577 worst_q_ratio=1.218
reference average sigma_overall=0.5045 worst_q_ratio=1.215
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465_astrometric_residuals.png (921 matched stars from wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176_astrometric_residuals.png (922 matched stars from wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096_astrometric_residuals.png (909 matched stars from wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097_astrometric_residuals.png (909 matched stars from wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits'
Saving fully-calibrated image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits'
Preparing the HTML report for the field Oph-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:17:54.90 -12:00:42.6: 10.95 +/- 0.01 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:17:54.90 -12:00:42.6: 11.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.01
Forced photometry filter KEPT candidate at 18:17:54.90 -12:00:42.6: ref_mag=10.97 +/- 0.01 new_mean_mag=10.0452 delta=0.92 (need > 0.90)
Adding exclusion_list_local.txt__out06468.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 10584_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 10584_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:34:15.26 -05:25:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06468_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 06468_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 02121_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 02121_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:35:33.39 -14:19:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02412_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 02412_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:12:38.25 -14:21:11.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Oph-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:17:54.90 -12:00:42.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
SExtractor catalog cache: saved Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat to cache
SExtractor catalog cache: saved Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
Creating symlink local_wcs_cache/wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits exists and is non-empty
wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits exists and is non-empty
wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits (1st reference image)
verification OK: wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
Image size: 937.8'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:00:09.727 -10:00:51.37 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/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_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits (1st new image)
verification OK: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
Image size: 942.1'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:00:01.471 -10:00:01.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:00:09.727 -10:00:51.37
Second-epoch image center 18:00:01.471 -10:00:01.34
Angular distance between the image centers 0.0366 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits (2nd new image)
verification OK: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Image size: 942.1'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 17:59:58.751 -10:00:39.19 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:00:09.727 -10:00:51.37
Second-epoch image center 17:59:58.751 -10:00:39.19
Angular distance between the image centers 0.0452 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 18:00:01.471 -10:00:01.34
Second-epoch second image center 17:59:58.751 -10:00:39.19
Angular distance between the image centers 0.01533 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits &> /tmp/tmp.ll2rkYrG6v
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.OueoIE5GrY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits &> /tmp/tmp.IJyZBDUpG4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits &> /tmp/tmp.1YEda4XW0y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.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_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits and wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits and wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
Found non-empty wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits and wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
The reference image (wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits) and catalog (wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat) found
'wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat' -> 'wcsmag.cat'
Read 92589 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 261.9134 to 278.0931 deg, Dec -15.2890 to -4.6853 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 261.9134 to 278.0931 deg, Dec -15.2890 to -4.6853 deg
Loaded 6353 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): 4652 out of 5614 total matches.
Matched with Tycho-2 5614 out of 92589 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.687800
a=0.000000 b=1.000000 c=22.687800
From vast_summary.log: estimated ref. image limiting mag.: -7.83
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.86
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 92589 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 261.9134 to 278.0931 deg, Dec -15.2890 to -4.6853 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 261.9134 to 278.0931 deg, Dec -15.2890 to -4.6853 deg
Loaded 6353 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): 4652 out of 5614 total matches.
Matched with Tycho-2 5614 out of 92589 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits:
Forced-photometry filter: calibrated wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits -> calib.txt_param_ref_wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits (aperture=4.8)
Read 81478 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 261.5495 to 278.2240 deg, Dec -15.6769 to -4.1775 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 261.5495 to 278.2240 deg, Dec -15.6769 to -4.1775 deg
Loaded 7384 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): 5031 out of 5872 total matches.
Matched with Tycho-2 5872 out of 81478 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: calibrated wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=4.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 123 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
2.0 pix Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
3.4 pix fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
3.4 pix fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
2.4 pix wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
2.0 pix wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Limiting magnitude estimates:
14.9 mag. Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
14.6 mag. Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
12.6 mag. fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
12.7 mag. fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ll2rkYrG6v (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits' -> 'wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
WCS_IMAGE_NAME=wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
WCS-calibrated image found: wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
Checking if the catalog wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat corresponding to the image wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits alredy exist and is non-empty...
Catalog wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat corresponding to the image wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits
WCS catalog name: wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=7825, passed=92581
Got 92581 stars (including 84614 good ones) from the SExtractor catalog wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat
util/solve_plate_with_UCAC5 got 92581 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 87871 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 87874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 87874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits N_match=928 sigma_overall_arcsec=0.590 sigma_q1_arcsec=0.487 sigma_q2_arcsec=0.786 sigma_q3_arcsec=0.540 sigma_q4_arcsec=0.526 n_q1=247 n_q2=386 n_q3=141 n_q4=154 worst_quadrant_to_overall_ratio=1.332
The image catalog is written to wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits -region wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OueoIE5GrY (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat corresponding to the image wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat corresponding to the image wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=5258, passed=81465
Got 81465 stars (including 76020 good ones) from the SExtractor catalog wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
util/solve_plate_with_UCAC5 got 81465 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.4'
Seting catalog search parameters based on the expected field of view 942.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013089 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010471 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 77711 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 77711 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 77711 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=934 sigma_overall_arcsec=0.392 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.415 sigma_q4_arcsec=0.432 n_q1=248 n_q2=387 n_q3=156 n_q4=143 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IJyZBDUpG4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
WCS_IMAGE_NAME=wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
WCS-calibrated image found: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
Checking if the catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat corresponding to the image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat corresponding to the image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
WCS catalog name: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=432, passed=13067
Got 13067 stars (including 12617 good ones) from the SExtractor catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat
util/solve_plate_with_UCAC5 got 13067 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 12498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 12496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 12496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits N_match=912 sigma_overall_arcsec=0.520 sigma_q1_arcsec=0.685 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.355 sigma_q4_arcsec=0.452 n_q1=224 n_q2=372 n_q3=162 n_q4=154 worst_quadrant_to_overall_ratio=1.318
The image catalog is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits -region wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1YEda4XW0y (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
WCS_IMAGE_NAME=wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
WCS-calibrated image found: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Checking if the catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat corresponding to the image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat corresponding to the image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
WCS catalog name: wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=452, passed=13565
Got 13565 stars (including 13095 good ones) from the SExtractor catalog wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat
util/solve_plate_with_UCAC5 got 13565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 12906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 12904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 12904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 911 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits N_match=911 sigma_overall_arcsec=0.545 sigma_q1_arcsec=0.686 sigma_q2_arcsec=0.576 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.524 n_q1=220 n_q2=385 n_q3=152 n_q4=154 worst_quadrant_to_overall_ratio=1.260
The image catalog is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits -region wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-50-31_20.00sec_-0.00C_LIGHTs_0096.fits
Saving fully-calibrated image wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Oph-06-Q1b1x1_235208_TTUQ1b1x1_2043487_ii1g7KJx/wcs_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097.fits
Preparing the HTML report for the field Oph-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:15:31.77 -14:11:01.3: 11.99 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:32:15.00 -13:37:37.5: 11.94 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:22:00.74 -06:57:49.0: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:32:15.00 -13:37:37.5: 11.81 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:15:31.77 -14:11:01.3: 12.20 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:22:00.74 -06:57:49.0: 15.20 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter REJECTED candidate at 18:15:31.77 -14:11:01.3: ref_mag=12.06 +/- 0.01 new_mean_mag=11.2826 delta=0.78 (need > 0.90)
Forced photometry filter REJECTED candidate at 17:32:15.00 -13:37:37.5: ref_mag=11.88 +/- 0.01 new_mean_mag=11.7438 delta=0.14 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:20:46.63 -10:25:50.8: 12.66 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:12:02.53 -13:02:57.6: 12.60 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:18:18.28 -12:10:56.9: 10.51 +/- 0.01 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:20:46.63 -10:25:50.8: 12.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry filter REJECTED candidate at 18:20:46.63 -10:25:50.8: ref_mag=12.68 +/- 0.02 new_mean_mag=11.7902 delta=0.89 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:09:46.63 -14:33:46.6: 12.87 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:18:18.28 -12:10:56.9: 10.40 +/- 0.01 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:12:02.53 -13:02:57.6: 12.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.46 +/- 0.00
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry filter KEPT candidate at 18:18:18.28 -12:10:56.9: ref_mag=10.46 +/- 0.00 new_mean_mag=9.5057 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 18:12:02.53 -13:02:57.6: ref_mag=12.62 +/- 0.02 new_mean_mag=11.5043 delta=1.12 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:11:23.07 -14:53:14.5: 12.91 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:39:47.55 -07:25:34.0: 13.15 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:09:46.63 -14:33:46.6: 12.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.03
Forced photometry filter KEPT candidate at 18:09:46.63 -14:33:46.6: ref_mag=12.87 +/- 0.03 new_mean_mag=11.8545 delta=1.01 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:31:33.03 -09:48:28.5: 12.70 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:11:23.07 -14:53:14.5: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.03
Forced photometry filter KEPT candidate at 18:11:23.07 -14:53:14.5: ref_mag=12.95 +/- 0.03 new_mean_mag=11.8913 delta=1.05 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:39:47.55 -07:25:34.0: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter KEPT candidate at 17:39:47.55 -07:25:34.0: ref_mag=13.08 +/- 0.03 new_mean_mag=12.1199 delta=0.96 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:31:33.03 -09:48:28.5: 12.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter KEPT candidate at 17:31:33.03 -09:48:28.5: ref_mag=12.64 +/- 0.02 new_mean_mag=11.5978 delta=1.04 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:08:14.74 -14:52:56.0: 13.29 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:08:14.74 -14:52:56.0: 13.45 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Forced photometry filter KEPT candidate at 18:08:14.74 -14:52:56.0: ref_mag=13.34 +/- 0.04 new_mean_mag=12.0763 delta=1.27 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:37:21.35 -07:02:36.5: 13.42 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:33:31.50 -07:12:54.8: 11.89 +/- 0.01 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:37:21.35 -07:02:36.5: 13.26 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.04
Forced photometry filter KEPT candidate at 17:37:21.35 -07:02:36.5: ref_mag=13.35 +/- 0.04 new_mean_mag=12.2851 delta=1.07 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:33:31.50 -07:12:54.8: 11.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry filter REJECTED candidate at 17:33:31.50 -07:12:54.8: ref_mag=11.83 +/- 0.01 new_mean_mag=11.0091 delta=0.82 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:41:46.67 -06:27:40.7: 12.61 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:41:46.67 -06:27:40.7: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Forced photometry filter KEPT candidate at 17:41:46.67 -06:27:40.7: ref_mag=12.52 +/- 0.02 new_mean_mag=10.9769 delta=1.54 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:19:01.00 -11:18:23.0: 13.44 +/- 0.06 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:13:52.99 -14:40:55.3: 12.92 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:21:09.30 -10:21:48.2: 12.65 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:19:01.00 -11:18:23.0: 13.51 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.05
Forced photometry filter KEPT candidate at 18:19:01.00 -11:18:23.0: ref_mag=13.46 +/- 0.05 new_mean_mag=12.1993 delta=1.27 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:17:02.91 -12:57:33.1: 13.42 +/- 0.06 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:21:09.30 -10:21:48.2: 13.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Forced photometry filter KEPT candidate at 18:21:09.30 -10:21:48.2: ref_mag=12.74 +/- 0.02 new_mean_mag=11.8013 delta=0.94 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:13:52.99 -14:40:55.3: 13.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.04
Forced photometry filter KEPT candidate at 18:13:52.99 -14:40:55.3: ref_mag=12.99 +/- 0.04 new_mean_mag=11.9078 delta=1.08 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:17:02.91 -12:57:33.1: 13.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Forced photometry filter KEPT candidate at 18:17:02.91 -12:57:33.1: ref_mag=13.38 +/- 0.05 new_mean_mag=12.2367 delta=1.15 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:18:01.22 -11:29:13.5: 13.40 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:11:30.94 -14:54:25.2: 12.65 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:18:01.22 -11:29:13.5: 13.54 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Forced photometry filter KEPT candidate at 18:18:01.22 -11:29:13.5: ref_mag=13.44 +/- 0.04 new_mean_mag=12.3265 delta=1.12 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:23:28.49 -08:54:07.4: 12.30 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:11:30.94 -14:54:25.2: 12.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter KEPT candidate at 18:11:30.94 -14:54:25.2: ref_mag=12.66 +/- 0.02 new_mean_mag=11.5375 delta=1.12 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:23:28.49 -08:54:07.4: 12.35 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:24:58.13 -10:46:08.8: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Forced photometry filter KEPT candidate at 18:23:28.49 -08:54:07.4: ref_mag=12.32 +/- 0.02 new_mean_mag=10.9640 delta=1.36 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:14:18.74 -14:11:16.8: 12.91 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:24:58.13 -10:46:08.8: 13.60 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.05
Forced photometry filter KEPT candidate at 18:24:58.13 -10:46:08.8: ref_mag=13.35 +/- 0.05 new_mean_mag=12.1427 delta=1.21 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:14:18.74 -14:11:16.8: 12.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Forced photometry filter KEPT candidate at 18:14:18.74 -14:11:16.8: ref_mag=12.91 +/- 0.03 new_mean_mag=11.9064 delta=1.00 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:15:03.15 -13:57:36.1: 12.27 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:15:03.15 -13:57:36.1: 12.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Forced photometry filter KEPT candidate at 18:15:03.15 -13:57:36.1: ref_mag=12.31 +/- 0.02 new_mean_mag=11.2492 delta=1.06 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:13:23.58 -15:02:58.7: 11.85 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:13:23.58 -15:02:58.7: 11.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry filter KEPT candidate at 18:13:23.58 -15:02:58.7: ref_mag=11.83 +/- 0.01 new_mean_mag=10.7147 delta=1.12 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:40:10.30 -07:30:54.7: 13.26 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:40:10.30 -07:30:54.7: 13.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Forced photometry filter KEPT candidate at 17:40:10.30 -07:30:54.7: ref_mag=13.22 +/- 0.04 new_mean_mag=12.2902 delta=0.93 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:09:53.77 -14:36:22.6: 12.24 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:09:53.77 -14:36:22.6: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Forced photometry filter KEPT candidate at 18:09:53.77 -14:36:22.6: ref_mag=12.23 +/- 0.02 new_mean_mag=11.2976 delta=0.93 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 17:32:25.58 -07:29:59.5: 12.54 +/- 0.03 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 17:32:25.58 -07:29:59.5: 12.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Forced photometry filter KEPT candidate at 17:32:25.58 -07:29:59.5: ref_mag=12.55 +/- 0.02 new_mean_mag=11.4615 delta=1.09 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:26:11.51 -07:43:43.7: 13.38 +/- 0.06 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:12:43.36 -14:53:11.5: 13.05 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:26:11.51 -07:43:43.7: 13.52 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.05
Forced photometry filter KEPT candidate at 18:26:11.51 -07:43:43.7: ref_mag=13.42 +/- 0.05 new_mean_mag=12.2760 delta=1.15 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:12:43.36 -14:53:11.5: 13.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.04
Forced photometry filter KEPT candidate at 18:12:43.36 -14:53:11.5: ref_mag=13.06 +/- 0.04 new_mean_mag=11.9321 delta=1.13 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:13:02.61 -12:16:36.0: 11.73 +/- 0.01 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:13:02.61 -12:16:36.0: 11.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Forced photometry filter KEPT candidate at 18:13:02.61 -12:16:36.0: ref_mag=11.63 +/- 0.01 new_mean_mag=10.6307 delta=1.00 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:19:19.44 -12:47:57.6: 14.01 +/- 0.10 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:26:36.94 -07:31:49.8: 13.02 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:26:36.94 -07:31:49.8: 13.05 +/- 0.06 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:19:19.44 -12:47:57.6: 13.96 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Forced photometry reference-image weighted average: 13.99 +/- 0.08
Forced photometry filter KEPT candidate at 18:26:36.94 -07:31:49.8: ref_mag=13.03 +/- 0.03 new_mean_mag=12.0326 delta=1.00 (need > 0.90)
Forced photometry filter KEPT candidate at 18:19:19.44 -12:47:57.6: ref_mag=13.99 +/- 0.08 new_mean_mag=12.3959 delta=1.60 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:24:09.52 -10:37:37.4: 12.16 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:24:09.52 -10:37:37.4: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Forced photometry filter KEPT candidate at 18:24:09.52 -10:37:37.4: ref_mag=12.23 +/- 0.02 new_mean_mag=11.2756 delta=0.96 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:12:31.56 -14:21:36.0: 12.80 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:12:31.56 -14:21:36.0: 12.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Forced photometry filter KEPT candidate at 18:12:31.56 -14:21:36.0: ref_mag=12.83 +/- 0.03 new_mean_mag=11.7619 delta=1.06 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:18:49.64 -12:30:44.7: 12.99 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:19:51.46 -12:04:09.1: 12.11 +/- 0.02 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:18:49.64 -12:30:44.7: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:19:51.46 -12:04:09.1: 12.26 +/- 0.03 detection
Forced photometry filter KEPT candidate at 18:18:49.64 -12:30:44.7: ref_mag=13.00 +/- 0.03 new_mean_mag=11.7105 delta=1.29 (need > 0.90)
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter KEPT candidate at 18:19:51.46 -12:04:09.1: ref_mag=12.15 +/- 0.01 new_mean_mag=11.1098 delta=1.05 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:08:46.70 -13:46:00.8: 12.99 +/- 0.04 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:08:46.70 -13:46:00.8: 12.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Forced photometry filter KEPT candidate at 18:08:46.70 -13:46:00.8: ref_mag=12.91 +/- 0.03 new_mean_mag=12.0000 delta=0.91 (need > 0.90)
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:24:12.30 -11:26:53.1: 13.00 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-03-21_05-22-41_20.00sec_-15.00C_LIGHT_0465.fits at 18:24:52.68 -08:36:53.9: 13.18 +/- 0.05 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:24:12.30 -11:26:53.1: 13.17 +/- 0.07 detection
Forced photometry on wcs_Oph-06-Q1b1x1_2026-04-10_02-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 18:24:52.68 -08:36:53.9: 13.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.04
Forced photometry filter KEPT candidate at 18:24:12.30 -11:26:53.1: ref_mag=13.05 +/- 0.04 new_mean_mag=11.9817 delta=1.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Forced photometry filter KEPT candidate at 18:24:52.68 -08:36:53.9: ref_mag=13.25 +/- 0.04 new_mean_mag=12.1821 delta=1.07 (need > 0.90)
Adding exclusion_list_local.txt__out03248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90977.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 39s
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: 20s
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Considering the candidate 111757_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111757_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
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Considering the candidate 111763_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111763_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
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Considering the candidate 111770_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111770_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:03.21 -14:48:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111774_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111774_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:06.35 -14:50:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111775_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111775_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:29:37.10 -14:44:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111776_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111776_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:24.66 -14:35:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111778_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 111778_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 111782_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111782_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:38.35 -15:02:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111784_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111784_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:29:26.75 -15:03:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111786_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111786_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:28.01 -15:07:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111787_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111787_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:03:10.40 -08:11:46.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 111795_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111795_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:28:32.55 -15:07:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111799_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111799_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:09.25 -15:05:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111803_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 111803_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:55:05.07 -12:53:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68756_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 68756_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:23:39.51 -08:56:05.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31372_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 31372_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:41:24.99 -12:52:32.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 59006_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 59006_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
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Considering the candidate 28515_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 28515_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:00:23.50 -13:17:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41694_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 41694_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 32053_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 32053_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 04651_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 04651_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:11:57.94 -14:57:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11055_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 11055_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 36048_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 36048_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:48:29.51 -12:40:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06227_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 06227_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 61491_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 61491_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:18:40.72 -10:04:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76379_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 76379_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 23882_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 23882_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:35:59.17 -13:32:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62675_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 62675_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 25811_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 25811_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:12:29.04 -13:31:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52894_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 52894_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:20:39.28 -11:08:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54368_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 54368_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:22:39.03 -10:57:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06345_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 06345_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 23954_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 23954_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:41:03.87 -13:35:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76795_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 76795_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:36.15 -07:11:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57925_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 57925_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:23:20.27 -10:32:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52170_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 52170_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:16:23.10 -11:13:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79381_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 79381_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 89300_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 89300_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
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Considering the candidate 78821_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 78821_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:37:38.01 -06:08:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07762_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 07762_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:13:24.23 -14:46:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75651_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 75651_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 88959_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 88959_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:09:30.52 -06:51:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34164_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 34164_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:33:44.10 -12:44:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92533_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 92533_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:32:22.44 -06:04:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36466_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 36466_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:05:58.53 -12:40:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84312_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 84312_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:37:59.78 -06:22:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51530_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 51530_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 43707_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 43707_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:17:54.95 -12:00:42.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 59469_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 59469_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 09350_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 09350_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 33303_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 33303_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 66201_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 66201_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:29:11.92 -09:26:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48029_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 48029_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:22:20.53 -11:33:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89989_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 89989_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:26:34.21 -08:26:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49823_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 49823_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 05834_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 05834_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 90076_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 90076_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:31:34.40 -08:18:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10550_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 10550_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:35:33.36 -14:19:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81167_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 81167_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 106261_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 106261_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:29:26.75 -09:35:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56123_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 56123_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 16319_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 16319_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 62308_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 62308_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:20:19.97 -09:59:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89028_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 89028_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:25:00.75 -06:50:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37183_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 37183_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:15:03.55 -12:37:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19585_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 19585_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 03248_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 03248_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 90647_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 90647_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:50.88 -08:29:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56611_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 56611_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:19:40.11 -10:42:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12375_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 12375_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:35:38.02 -14:16:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78098_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 78098_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:30:28.66 -06:58:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90983_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 90983_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:32:47.45 -08:22:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50213_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 50213_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:30:29.54 -11:18:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13448_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 13448_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:12:38.26 -14:21:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77803_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 77803_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 68838_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 68838_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:17.66 -09:03:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29783_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 29783_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:05:47.56 -13:11:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02883_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 02883_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:12:20.01 -15:05:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10400_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 10400_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 11520_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 11520_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:11:32.39 -14:28:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78151_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 78151_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
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Considering the candidate 49515_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 49515_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:07:04.74 -11:30:51.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83463_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 83463_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:36:01.70 -06:32:05.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72027_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 72027_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:48:17.96 -05:14:08.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79232_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 79232_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06195_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 06195_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54671_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 54671_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:16:28.67 -10:55:52.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26810_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 26810_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:16:43.15 -13:25:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52025_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 52025_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:24:11.10 -11:12:39.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40941_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 40941_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29212_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 29212_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:05:31.52 -13:16:34.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07017_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 07017_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:14:02.91 -14:49:34.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35235_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 35235_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76736_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 76736_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29553_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 29553_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:05:27.26 -13:14:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05831_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 05831_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:11:55.01 -14:52:58.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41495_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 41495_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:19:43.60 -12:13:16.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56784_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 56784_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58224_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 58224_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:13:13.84 -10:28:22.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73110_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 73110_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:37:19.34 -05:23:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13900_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 13900_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73349_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 73349_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:34:15.28 -05:25:57.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61985_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 61985_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:21:41.70 -10:02:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104373_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 104373_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:38:14.27 -04:38:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28541_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 28541_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:16:11.69 -13:18:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90256_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 90256_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:09:20.65 -08:29:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03961_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 03961_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:13:43.89 -15:02:14.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38414_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 38414_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43397_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 43397_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59919_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 59919_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:26:34.17 -10:17:31.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22409_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 22409_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85885_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 85885_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:30:11.09 -08:11:18.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79625_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 79625_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:28:48.06 -07:44:26.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14871_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 14871_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:30:59.95 -14:07:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70951_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 70951_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:38:34.57 -04:59:28.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49971_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 49971_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90977_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
Preparing report for the candidate 90977_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40790_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 40790_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:18:55.23 -12:18:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62563_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 62563_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:59:01.59 -09:46:32.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92184_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 92184_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:36:32.72 -05:47:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85888_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 85888_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:03:04.89 -08:10:55.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18895_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 18895_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 18:09:43.38 -13:56:04.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85975_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097
The candidate 85975_fd_Oph-06-Q1b1x1_2026-05-25_23-51-19_20.00sec_0.00C_LIGHTs_0097 did not pass the final checks
**** FOUND 17:37:50.89 -08:07:10.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 61s
Prepared the HTML report for the field Oph-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:17:54.90 -12:00:42.6
18:13:23.58 -15:02:58.7
18:11:30.94 -14:54:25.2
18:12:43.36 -14:53:11.5
18:11:23.07 -14:53:14.5
18:08:14.74 -14:52:56.0
18:13:52.99 -14:40:55.3
18:09:53.77 -14:36:22.6
18:09:46.63 -14:33:46.6
18:22:00.74 -06:57:49.0
18:12:31.56 -14:21:36.0
18:14:18.74 -14:11:16.8
18:15:03.15 -13:57:36.1
18:08:46.70 -13:46:00.8
18:12:02.53 -13:02:57.6
18:17:02.91 -12:57:33.1
18:19:19.44 -12:47:57.6
18:18:49.64 -12:30:44.7
18:13:02.61 -12:16:36.0
18:18:18.28 -12:10:56.9
18:19:51.46 -12:04:09.1
18:18:01.22 -11:29:13.5
18:24:12.30 -11:26:53.1
18:19:01.00 -11:18:23.0
18:24:58.13 -10:46:08.8
18:24:09.52 -10:37:37.4
18:21:09.30 -10:21:48.2
17:31:33.03 -09:48:28.5
17:41:46.67 -06:27:40.7
17:39:47.55 -07:25:34.0
18:26:36.94 -07:31:49.8
17:40:10.30 -07:30:54.7
17:32:25.58 -07:29:59.5
18:26:11.51 -07:43:43.7
17:37:21.35 -07:02:36.5
18:23:28.49 -08:54:07.4
18:24:52.68 -08:36:53.9
########### Completed Oph-06-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
18:17:54.90 -12:00:42.6
18:22:00.74 -06:57:49.0
18:18:18.28 -12:10:56.9
18:12:02.53 -13:02:57.6
18:09:46.63 -14:33:46.6
18:11:23.07 -14:53:14.5
17:39:47.55 -07:25:34.0
17:31:33.03 -09:48:28.5
18:08:14.74 -14:52:56.0
17:37:21.35 -07:02:36.5
17:41:46.67 -06:27:40.7
18:19:01.00 -11:18:23.0
18:21:09.30 -10:21:48.2
18:13:52.99 -14:40:55.3
18:17:02.91 -12:57:33.1
18:18:01.22 -11:29:13.5
18:11:30.94 -14:54:25.2
18:23:28.49 -08:54:07.4
18:24:58.13 -10:46:08.8
18:14:18.74 -14:11:16.8
18:15:03.15 -13:57:36.1
18:13:23.58 -15:02:58.7
17:40:10.30 -07:30:54.7
18:09:53.77 -14:36:22.6
17:32:25.58 -07:29:59.5
18:26:11.51 -07:43:43.7
18:12:43.36 -14:53:11.5
18:13:02.61 -12:16:36.0
18:19:19.44 -12:47:57.6
18:26:36.94 -07:31:49.8
18:24:09.52 -10:37:37.4
18:12:31.56 -14:21:36.0
18:18:49.64 -12:30:44.7
18:19:51.46 -12:04:09.1
18:08:46.70 -13:46:00.8
18:24:12.30 -11:26:53.1
18:24:52.68 -08:36:53.9
###################################################################################
18:17:54.90 -12:00:42.6 -- not an asteroid (will add it to exclusion list)
18:22:00.74 -06:57:49.0 -- asteroid (will NOT add it to exclusion list)
18:18:18.28 -12:10:56.9 -- not an asteroid (will add it to exclusion list)
18:12:02.53 -13:02:57.6 -- not an asteroid (will add it to exclusion list)
18:09:46.63 -14:33:46.6 -- not an asteroid (will add it to exclusion list)
18:11:23.07 -14:53:14.5 -- not an asteroid (will add it to exclusion list)
17:39:47.55 -07:25:34.0 -- not an asteroid (will add it to exclusion list)
17:31:33.03 -09:48:28.5 -- not an asteroid (will add it to exclusion list)
18:08:14.74 -14:52:56.0 -- not an asteroid (will add it to exclusion list)
17:37:21.35 -07:02:36.5 -- not an asteroid (will add it to exclusion list)
17:41:46.67 -06:27:40.7 -- not an asteroid (will add it to exclusion list)
18:19:01.00 -11:18:23.0 -- asteroid (will NOT add it to exclusion list)
18:21:09.30 -10:21:48.2 -- not an asteroid (will add it to exclusion list)
18:13:52.99 -14:40:55.3 -- not an asteroid (will add it to exclusion list)
18:17:02.91 -12:57:33.1 -- not an asteroid (will add it to exclusion list)
18:18:01.22 -11:29:13.5 -- not an asteroid (will add it to exclusion list)
18:11:30.94 -14:54:25.2 -- not an asteroid (will add it to exclusion list)
18:23:28.49 -08:54:07.4 -- asteroid (will NOT add it to exclusion list)
18:24:58.13 -10:46:08.8 -- not an asteroid (will add it to exclusion list)
18:14:18.74 -14:11:16.8 -- not an asteroid (will add it to exclusion list)
18:15:03.15 -13:57:36.1 -- not an asteroid (will add it to exclusion list)
18:13:23.58 -15:02:58.7 -- not an asteroid (will add it to exclusion list)
17:40:10.30 -07:30:54.7 -- not an asteroid (will add it to exclusion list)
18:09:53.77 -14:36:22.6 -- not an asteroid (will add it to exclusion list)
17:32:25.58 -07:29:59.5 -- asteroid (will NOT add it to exclusion list)
18:26:11.51 -07:43:43.7 -- not an asteroid (will add it to exclusion list)
18:12:43.36 -14:53:11.5 -- not an asteroid (will add it to exclusion list)
18:13:02.61 -12:16:36.0 -- not an asteroid (will add it to exclusion list)
18:19:19.44 -12:47:57.6 -- not an asteroid (will add it to exclusion list)
18:26:36.94 -07:31:49.8 -- not an asteroid (will add it to exclusion list)
18:24:09.52 -10:37:37.4 -- not an asteroid (will add it to exclusion list)
18:12:31.56 -14:21:36.0 -- not an asteroid (will add it to exclusion list)
18:18:49.64 -12:30:44.7 -- not an asteroid (will add it to exclusion list)
18:19:51.46 -12:04:09.1 -- not an asteroid (will add it to exclusion list)
18:08:46.70 -13:46:00.8 -- not an asteroid (will add it to exclusion list)
18:24:12.30 -11:26:53.1 -- not an asteroid (will add it to exclusion list)
18:24:52.68 -08:36:53.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
17:31:33.03 -09:48:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:37:21.35 -07:02:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:39:47.55 -07:25:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:40:10.30 -07:30:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:41:46.67 -06:27:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:08:14.74 -14:52:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:08:46.70 -13:46:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:09:46.63 -14:33:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:09:53.77 -14:36:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:23.07 -14:53:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:30.94 -14:54:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:12:02.53 -13:02:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:12:31.56 -14:21:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:12:43.36 -14:53:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:13:02.61 -12:16:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:13:23.58 -15:02:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:13:52.99 -14:40:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:14:18.74 -14:11:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:03.15 -13:57:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:02.91 -12:57:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:54.90 -12:00:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:01.22 -11:29:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:18.28 -12:10:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:49.64 -12:30:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:19.44 -12:47:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:51.46 -12:04:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:09.30 -10:21:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:09.52 -10:37:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:12.30 -11:26:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:52.68 -08:36:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:58.13 -10:46:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:11.51 -07:43:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:36.94 -07:31:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
17:31:33.03 -09:48:28.5 -- a known variable star
17:37:21.35 -07:02:36.5 -- not a known variable star
17:39:47.55 -07:25:34.0 -- a known variable star
17:40:10.30 -07:30:54.7 -- a known variable star
17:41:46.67 -06:27:40.7 -- a known variable star
18:08:14.74 -14:52:56.0 -- a known variable star
18:08:46.70 -13:46:00.8 -- a known variable star
18:09:46.63 -14:33:46.6 -- a known variable star
18:09:53.77 -14:36:22.6 -- a known variable star
18:11:23.07 -14:53:14.5 -- a known variable star
18:11:30.94 -14:54:25.2 -- not a known variable star
18:12:02.53 -13:02:57.6 -- a known variable star
18:12:31.56 -14:21:36.0 -- not a known variable star
18:12:43.36 -14:53:11.5 -- a known variable star
18:13:02.61 -12:16:36.0 -- a known variable star
18:13:23.58 -15:02:58.7 -- a known variable star
18:13:52.99 -14:40:55.3 -- not a known variable star
18:14:18.74 -14:11:16.8 -- not a known variable star
18:15:03.15 -13:57:36.1 -- not a known variable star
18:17:02.91 -12:57:33.1 -- not a known variable star
18:17:54.90 -12:00:42.6 -- a known variable star
18:18:01.22 -11:29:13.5 -- not a known variable star
18:18:18.28 -12:10:56.9 -- a known variable star
18:18:49.64 -12:30:44.7 -- a known variable star
18:19:19.44 -12:47:57.6 -- a known variable star
18:19:51.46 -12:04:09.1 -- a known variable star
18:21:09.30 -10:21:48.2 -- a known variable star
18:24:09.52 -10:37:37.4 -- a known variable star
18:24:12.30 -11:26:53.1 -- a known variable star
18:24:52.68 -08:36:53.9 -- a known variable star
18:24:58.13 -10:46:08.8 -- a known variable star
18:26:11.51 -07:43:43.7 -- a known variable star
18:26:36.94 -07:31:49.8 -- a known variable star
Found 8 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
33 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
17:31:33.03 -09:48:28.5
17:37:21.35 -07:02:36.5
17:39:47.55 -07:25:34.0
17:40:10.30 -07:30:54.7
17:41:46.67 -06:27:40.7
18:08:14.74 -14:52:56.0
18:08:46.70 -13:46:00.8
18:09:46.63 -14:33:46.6
18:09:53.77 -14:36:22.6
18:11:23.07 -14:53:14.5
18:11:30.94 -14:54:25.2
18:12:02.53 -13:02:57.6
18:12:31.56 -14:21:36.0
18:12:43.36 -14:53:11.5
18:13:02.61 -12:16:36.0
18:13:23.58 -15:02:58.7
18:13:52.99 -14:40:55.3
18:14:18.74 -14:11:16.8
18:15:03.15 -13:57:36.1
18:17:02.91 -12:57:33.1
18:17:54.90 -12:00:42.6
18:18:01.22 -11:29:13.5
18:18:18.28 -12:10:56.9
18:18:49.64 -12:30:44.7
18:19:19.44 -12:47:57.6
18:19:51.46 -12:04:09.1
18:21:09.30 -10:21:48.2
18:24:09.52 -10:37:37.4
18:24:12.30 -11:26:53.1
18:24:52.68 -08:36:53.9
18:24:58.13 -10:46:08.8
18:26:11.51 -07:43:43.7
18:26:36.94 -07:31:49.8
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461186.70187311 -observatory V36
05:07:21.94 +24:43:31.0 Mercury (-1.1mag)
06:36:00.04 +24:58:56.5 Venus (-3.9mag)
02:12:06.35 +12:34:09.2 Mars (1.3mag)
07:37:59.99 +21:56:23.8 Jupiter (-1.9mag)
00:45:18.41 +02:25:55.1 Saturn (0.9mag)
03:57:04.41 +20:16:19.6 Uranus (5.8mag)
00:15:13.81 +00:11:34.2 Neptune (7.8mag)
20:33:56.23 -23:00:04.2 Pluto (14.5mag)
12:20:16.31 -05:52:54.0 Moon (-11.2mag)
-rw-r--r-- 1 apache apache 363 May 25 23:55 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461186.70187311:
07:37:54.98 +21:56:36.4 Io (5.9mag)
07:38:10.43 +21:55:54.0 Europa (6.1mag)
07:37:53.06 +21:56:48.1 Ganymede (5.5mag)
07:37:38.13 +21:57:17.3 Callisto (6.7mag)
07:39:05.04 +21:32:44.3 Himalia (15.5mag)
07:38:00.78 +21:56:23.0 Thebe (16.5mag)
07:39:23.38 +21:53:59.3 Elara (17.5mag)
07:39:27.85 +22:15:08.4 Pasiphae (17.7mag)
07:45:07.07 +21:57:13.4 Carme (18.8mag)
00:45:20.62 +02:25:35.3 Titan (8.7mag)
00:45:14.39 +02:26:02.8 Rhea (10.0mag)
00:45:41.12 +02:26:02.1 Iapetus (11.4mag)
00:45:33.14 +02:25:58.0 Hyperion (14.7mag)
00:46:16.03 +02:29:41.9 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 25 23:55 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461186.70187311:
17:17:22.53 -33:20:59.7 JWST
16:05:22.00 +52:05:30.5 Chandra
08:21:50.55 -45:17:19.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 25 23:55 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461186.70187311 -observatory V36
13:20:45.95 -27:03:30.0 14.4mag D/1884 O1 (Barnard)
06:37:24.31 +30:40:17.5 15.7mag D/1886 K1 (Brooks)
15:26:16.63 +01:21:00.6 14.6mag D/1895 Q1 (Swift)
05:28:12.57 +24:38:57.0 17.2mag D/1918 W1 (Schorr)
09:31:30.27 +14:31:45.4 17.9mag P/2009 WX51 (Catalina)
18:51:00.53 -31:39:31.5 13.7mag P/2010 H2 (Vales)
05:40:54.13 -68:16:01.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:21.75 +31:48:30.8 17.4mag C/2017 K2 (PANSTARRS)
17:19:51.23 +14:33:01.6 17.7mag C/2021 G2 (ATLAS)
23:14:32.77 +31:02:52.5 17.2mag C/2022 E2 (ATLAS)
05:18:02.00 +26:51:29.3 16.4mag C/2022 N2 (PANSTARRS)
09:20:58.52 +31:29:34.2 16.5mag C/2022 QE78 (ATLAS)
08:44:01.64 +03:13:10.8 17.6mag C/2022 R6 (PANSTARRS)
18:36:21.02 +21:12:19.6 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:26.50 -11:02:15.9 17.5mag P/2023 B1 (PANSTARRS)
22:16:12.46 +65:39:50.5 17.7mag C/2023 H5 (Lemmon)
18:17:03.53 -05:32:15.0 13.7mag C/2023 R1 (PANSTARRS)
13:39:43.93 +85:47:48.0 17.9mag C/2023 X2 (Lemmon)
06:53:27.49 +63:55:44.0 17.6mag C/2024 A1 (ATLAS)
06:26:55.14 +26:29:02.0 13.1mag C/2024 E1 (Wierzchos)
15:47:52.00 +12:12:40.9 17.3mag C/2024 G6 (ATLAS)
20:19:47.47 +27:10:48.7 14.1mag C/2024 J3 (ATLAS)
04:05:00.14 -17:12:07.2 16.1mag C/2024 T5 (ATLAS)
05:53:40.72 +36:48:41.0 17.9mag C/2025 J1 (Borisov)
11:45:40.13 +53:20:10.7 16.9mag C/2025 L1 (ATLAS)
06:24:57.69 -10:11:22.7 12.6mag C/2025 R3 (PANSTARRS)
12:40:57.00 +04:37:00.1 17.2mag C/2025 Y1 (ATLAS)
01:36:21.39 +42:23:02.5 15.7mag C/2026 B2 (Sun-Gao)
11:10:26.43 -08:58:43.0 16.3mag A/2026 E1
19:59:42.39 -08:07:25.5 9.5mag 10P/Tempel
14:18:44.90 -02:35:35.0 17.6mag 24P/Schaumasse
10:59:43.29 -00:51:55.2 15.9mag 29P/Schwassmann-Wachmann
10:51:19.96 -02:34:28.7 17.8mag 43P/Wolf-Harrington
02:51:29.49 +23:50:20.2 17.6mag 47P/Ashbrook-Jackson
08:32:17.29 +27:21:46.8 16.9mag 63P/Wild
00:14:54.27 -07:19:14.3 15.7mag 65P/Gunn
06:01:42.37 +31:41:18.8 16.5mag 76P/West-Kohoutek-Ikemura
02:38:00.73 +15:23:36.1 13.9mag 78P/Gehrels
00:51:12.02 +01:49:28.7 15.3mag 88P/Howell
04:12:50.15 +28:56:50.2 15.1mag 93P/Lovas
02:07:28.13 +25:21:25.3 17.9mag 114P/Wiseman-Skiff
06:20:02.39 +33:19:27.0 15.7mag 123P/West-Hartley
09:27:59.43 +20:15:37.8 16.4mag 124P/Mrkos
03:37:38.15 +18:17:27.5 16.4mag 128P/Shoemaker-Holt
04:07:36.71 +18:20:58.8 17.7mag 131P/Mueller
04:58:47.97 +19:38:40.1 13.0mag 141P/Machholz
05:01:26.63 +16:23:06.2 12.9mag 141P-A/Machholz
03:46:37.42 +13:43:22.6 10.6mag 141P-D/Machholz
02:48:12.75 -26:39:01.5 17.3mag 161P/Hartley-IRAS
02:59:57.72 +18:14:29.8 14.9mag 162P/SidingSpring
19:34:45.35 -01:42:23.9 17.6mag 169P/NEAT
17:02:20.36 -09:21:26.4 16.2mag 235P/LINEAR
07:05:04.74 +35:51:51.6 17.3mag 240P/NEAT
23:58:36.29 -07:45:46.1 16.7mag 260P/McNaught
03:30:03.27 +29:55:36.9 17.7mag 295P/LINEAR
22:05:26.76 -27:28:54.9 17.7mag 320P/McNaught
15:21:44.11 +08:21:36.7 17.4mag 391P/Kowalski
07:57:14.03 +21:02:17.6 17.8mag 450P/LONEOS
06:38:47.42 +42:35:09.6 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 25 23:55 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
-rw-r--r-- 1 apache apache 5.6K May 25 23:55 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
-rw-r--r-- 1 apache apache 188K May 25 23:55 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:51:00.147 -40:59:30.34 AT 2026myv 2026-05-04.40 19.85
23:01:42.557 -37:41:28.08 AT 2026myu 2026-05-14.36 20.03
17:40:41.796 +55:46:35.59 AT 2026myt 2026-05-13.08 19.76
11:57:21.623 +08:17:50.60 AT 2026mys 2026-05-17.92 20.12
18:08:09.175 +24:46:16.68 AT 2026myr 2026-05-16.11 19.59
19:44:08.720 +05:58:44.85 AT 2026myq 2026-05-18.09 19.96
22:15:03.694 +37:18:03.97 SN 2026myp 2026-05-17.58 17.878
13:28:54.990 -05:49:13.50 AT 2026myo 2026-05-17.76 18.69
13:35:39.060 +60:25:07.59 AT 2026myn 2026-05-17.79 18.94
15:11:37.375 +27:04:22.10 AT 2026mym 2026-05-17.80 19.01
15:45:32.128 +08:10:41.12 AT 2026myl 2026-05-17.84 19.27
16:38:47.743 +40:50:56.52 AT 2026myk 2026-05-17.88 18.14
13:21:16.033 -33:01:10.62 AT 2026myj 2026-05-10.44 20.34
14:04:07.440 +19:21:36.43 AT 2026myi 2026-05-16.96 20.28
12:09:08.262 +13:15:11.92 AT 2026myh 2026-05-05.92 20.33
17:37:21.286 +36:24:32.57 AT 2026myg 2026-05-12.55 19.89
14:40:52.425 +10:22:25.10 AT 2026myf 2026-05-14.32 20.45
21:41:13.013 +64:08:54.76 AT 2026mye 2026-05-17.15 19.242
17:07:33.400 +35:38:40.42 AT 2026myd 2026-05-17.43 20.44
20:38:48.864 -58:53:21.28 AT 2026myc 2026-05-13.27 19.093
-rw-r--r-- 1 apache apache 30K May 25 23:55 tns_transients_list.txt
