This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW
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 26.1289 2461186.6289 11.39 08:03:36.22 -05:09:49.5
226.05376 13.50176 galactic Mon Second-epoch detections are separated by 1.9" and 7.8 pix
The object was found in VSX14" Gaia DR3 3067486915781605120
Type: ROT
# Max. Min./Amp. JD0 Period
12.990 G 13.010 G G
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:36.22 -05:09:49.5: 12.29 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:36.22 -05:09:49.5: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067486915781605120,2461186.6289,11.39,0.05,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 3067486915781605120 20260526.1289 11.39CV 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 26.1289 2461186.6289 11.69 08:03:48.10 -06:05:55.6
226.91407 13.08259 galactic Mon Second-epoch detections are separated by 5.0" and 7.5 pix
The object was found in VSX 1" Gaia DR3 3067090090862867072
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.520 G 12.550 G 0.017474300000 A
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:48.10 -06:05:55.6: 12.65 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:48.10 -06:05:55.6: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067090090862867072,2461186.6289,11.69,0.05,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 3067090090862867072 20260526.1289 11.69CV 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 26.1289 2461186.6289 11.63 08:04:17.44 -05:47:55.0
226.70810 13.33691 galactic Mon Second-epoch detections are separated by 2.1" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3067376822879694208 | 08:04:17.50 -05:47:55.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.625+/-0.030 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:17.44 -05:47:55.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:17.44 -05:47:55.0: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067376822879694208,2461186.6289,11.63,0.05,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 3067376822879694208 20260526.1289 11.63CV 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 26.1289 2461186.6289 11.43 08:03:58.52 -04:57:18.2
225.91377 13.68507 galactic Mon Second-epoch detections are separated by 0.9" and 7.7 pix
The object was found in VSX 1" ASASSN-V J080358.44-045717.7
Type: SR
# Max. Min./Amp. JD0 Period
13.470 g Y 0.210 g 2458157.68800 43.810000000000
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:58.52 -04:57:18.2: 12.32 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:58.52 -04:57:18.2: 12.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J080358.44-045717.7,2461186.6289,11.43,0.05,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 J080358.44-045717.7 20260526.1289 11.43CV 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 26.1289 2461186.6289 11.58 08:04:56.44 -06:34:04.1
227.47633 13.09517 galactic Mon Second-epoch detections are separated by 2.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3067007352612909184 | 08:04:56.41 -06:34:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:56.44 -06:34:04.1: 12.60 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:56.44 -06:34:04.1: 12.65 +/- 0.03 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!
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 3067007352612909184,2461186.6289,11.58,0.05,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 3067007352612909184 20260526.1289 11.58CV 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 26.1289 2461186.6289 10.56 08:07:48.71 -05:03:21.9
226.49082 14.46599 galactic Mon Second-epoch detections are separated by 1.1" and 7.6 pix
The object was found in VSX 2" ASAS J080749-0503.4
Type: MISC
# Max. Min./Amp. JD0 Period
8.586 Ic Y 0.215 Ic 2452538.50000 63.950000000000
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:07:48.71 -05:03:21.9: 11.79 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:07:48.71 -05:03:21.9: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J080749-0503.4,2461186.6289,10.56,0.05,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 J080749-0503.4 20260526.1289 10.56CV 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 26.1289 2461186.6289 10.96 08:05:31.23 -06:01:48.6
227.07074 13.48761 galactic Mon Second-epoch detections are separated by 1.2" and 7.5 pix
The object was found in VSX 3" ASAS J080531-0601.8
Type: MISC
# Max. Min./Amp. JD0 Period
12.210 V Y 1.010 V 2452372.00000 185.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:05:31.23 -06:01:48.6: 12.29 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:05:31.23 -06:01:48.6: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J080531-0601.8,2461186.6289,10.96,0.05,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 J080531-0601.8 20260526.1289 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1289 2461186.6289 11.56 08:04:22.23 -06:18:43.2
227.17615 13.09953 galactic Mon Second-epoch detections are separated by 1.4" and 7.6 pix
The object was found in VSX 1" Gaia DR3 3067067722673198336
Type: VAR
# Max. Min./Amp. JD0 Period
12.260 G 12.270 G 0.014756800000 K
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:22.23 -06:18:43.2: 12.56 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:22.23 -06:18:43.2: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067067722673198336,2461186.6289,11.56,0.05,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 3067067722673198336 20260526.1289 11.56CV 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 26.1289 2461186.6289 11.61 08:07:31.79 -06:37:09.2
227.85207 13.62664 galactic Mon Second-epoch detections are separated by 1.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3064086293816974848 | 08:07:31.84 -06:37:07.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.658+/-0.033 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:07:31.79 -06:37:09.2: 12.56 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:07:31.79 -06:37:09.2: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3064086293816974848,2461186.6289,11.61,0.05,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 3064086293816974848 20260526.1289 11.61CV 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 26.1289 2461186.6289 11.62 08:04:41.13 -06:31:46.4
227.40988 13.05925 galactic Mon Second-epoch detections are separated by 1.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3067011308282833408 | 08:04:41.16 -06:31:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.642+/-0.034 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:41.13 -06:31:46.4: 12.54 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:41.13 -06:31:46.4: 12.55 +/- 0.02 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
Gaia DR3 3067011308282833408,2461186.6289,11.62,0.05,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 3067011308282833408 20260526.1289 11.62CV 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 26.1289 2461186.6289 11.95 08:04:20.80 -05:59:02.0
226.88057 13.25721 galactic Mon Second-epoch detections are separated by 2.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:04:20.80 -05:59:02.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.694+/-0.030 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:20.80 -05:59:02.0: 12.94 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:20.80 -05:59:02.0: 12.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.93 +/- 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
target,2461186.6289,11.95,0.05,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
target 20260526.1289 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 26.1289 2461186.6289 11.24 08:05:21.27 -05:46:38.9
226.82404 13.57721 galactic Mon Second-epoch detections are separated by 1.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3067195991875578368 | 08:05:21.23 -05:46:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.827+/-0.030 (M)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:05:21.27 -05:46:38.9: 12.16 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:05:21.27 -05:46:38.9: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067195991875578368,2461186.6289,11.24,0.05,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
Gaia DR3 3067195991875578368 20260526.1289 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 26.1289 2461186.6289 11.14 08:03:36.32 -06:18:15.5
227.07242 12.93830 galactic Mon Second-epoch detections are separated by 1.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3067077274680464256 | 08:03:36.27 -06:18:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.725+/-0.031 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:36.32 -06:18:15.5: 12.17 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:36.32 -06:18:15.5: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067077274680464256,2461186.6289,11.14,0.05,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 3067077274680464256 20260526.1289 11.14CV 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 26.1289 2461186.6289 11.92 08:06:18.26 -06:11:57.4
227.32133 13.57251 galactic Mon Second-epoch detections are separated by 2.5" and 8.1 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 | target | 08:06:18.26 -06:11:57.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.417+/-0.034 (G)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:06:18.26 -06:11:57.4: 12.90 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:06:18.26 -06:11:57.4: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 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
target,2461186.6289,11.92,0.05,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
target 20260526.1289 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1289 2461186.6289 11.52 08:06:04.66 -06:34:40.3
227.62989 13.33495 galactic Mon Second-epoch detections are separated by 1.1" and 7.7 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 J121.5192-06.5782 | 08:06:04.61 -06:34:41.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.014+/-0.033 (M)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:06:04.66 -06:34:40.3: 12.47 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:06:04.66 -06:34:40.3: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J121.5192-06.5782,2461186.6289,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J121.5192-06.5782 20260526.1289 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1289 2461186.6289 11.20 08:03:35.79 -06:21:59.1
227.12663 12.90558 galactic Mon Second-epoch detections are separated by 1.8" and 7.9 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 3067064703316335488 | 08:03:35.78 -06:22:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.782+/-0.034 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:35.79 -06:21:59.1: 12.11 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:35.79 -06:21:59.1: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067064703316335488,2461186.6289,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3067064703316335488 20260526.1289 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1289 2461186.6289 11.87 08:04:37.04 -06:03:02.5
226.97446 13.28251 galactic Mon Second-epoch detections are separated by 1.3" and 7.7 pix
The object was found in VSX 1" Gaia DR3 3067181011029717376
Type: ROT
# Max. Min./Amp. JD0 Period
12.660 G 12.680 G G
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:37.04 -06:03:02.5: 12.88 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:37.04 -06:03:02.5: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067181011029717376,2461186.6289,11.87,0.05,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
Gaia DR3 3067181011029717376 20260526.1289 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 26.1289 2461186.6289 11.88 08:03:53.96 -06:16:21.4
227.08138 13.01746 galactic Mon Second-epoch detections are separated by 3.8" and 7.2 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 | Gaia DR3 3067071609623683712 | 08:03:53.92 -06:16:19.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.652+/-0.031 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:53.96 -06:16:21.4: 12.86 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:53.96 -06:16:21.4: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067071609623683712,2461186.6289,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3067071609623683712 20260526.1289 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1289 2461186.6289 11.20 08:05:17.75 -06:22:33.1
227.35048 13.26725 galactic Mon Second-epoch detections are separated by 0.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3067020138735474304 | 08:05:17.88 -06:22:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G9 (LAMOST DR5) J-Ks=0.701+/-0.035 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:05:17.75 -06:22:33.1: 12.13 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:05:17.75 -06:22:33.1: 12.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067020138735474304,2461186.6289,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3067020138735474304 20260526.1289 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1289 2461186.6289 11.93 08:03:57.94 -05:16:46.9
226.20320 13.52303 galactic Mon Second-epoch detections are separated by 2.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:03:57.94 -05:16:46.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.333+/-0.035 (G)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:57.94 -05:16:46.9: 12.86 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:57.94 -05:16:46.9: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 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
target,2461186.6289,11.93,0.05,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
target 20260526.1289 11.93CV 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 26.1289 2461186.6289 11.81 08:04:04.06 -05:26:25.2
226.35977 13.46583 galactic Mon Second-epoch detections are separated by 2.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3067430806328873600 | 08:04:04.13 -05:26:26.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=0.899+/-0.041 (M)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:04.06 -05:26:25.2: 12.85 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:04.06 -05:26:25.2: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067430806328873600,2461186.6289,11.81,0.05,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 3067430806328873600 20260526.1289 11.81CV 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 26.1289 2461186.6289 11.95 08:05:18.89 -06:32:33.5
227.50146 13.18829 galactic Mon Second-epoch detections are separated by 3.3" and 7.6 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 | target | 08:05:18.89 -06:32:33.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:05:18.89 -06:32:33.5: 13.11 +/- 0.04 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:05:18.89 -06:32:33.5: 13.05 +/- 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
target,2461186.6289,11.95,0.05,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
target 20260526.1289 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 26.1289 2461186.6289 11.03 08:04:09.43 -06:24:29.9
227.23492 13.00568 galactic Mon Second-epoch detections are separated by 1.8" and 7.9 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 3067060782006055296 | 08:04:09.50 -06:24:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.251+/-0.033 (F)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:09.43 -06:24:29.9: 11.99 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:09.43 -06:24:29.9: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067060782006055296,2461186.6289,11.03,0.05,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 3067060782006055296 20260526.1289 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1289 2461186.6289 11.37 08:03:29.68 -05:24:44.6
226.26243 13.35559 galactic Mon Second-epoch detections are separated by 0.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3067455163084043776 | 08:03:29.74 -05:24:43.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.655+/-0.033 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:29.68 -05:24:44.6: 12.39 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:29.68 -05:24:44.6: 12.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3067455163084043776,2461186.6289,11.37,0.05,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 3067455163084043776 20260526.1289 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1289 2461186.6289 11.43 08:04:21.16 -05:50:08.4
226.74904 13.33195 galactic Mon Second-epoch detections are separated by 0.4" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J121.0883-05.8329 | 08:04:21.18 -05:50:07.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.600+/-0.033 (K)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:21.16 -05:50:08.4: 12.37 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:21.16 -05:50:08.4: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J121.0883-05.8329,2461186.6289,11.43,0.05,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 J121.0883-05.8329 20260526.1289 11.43CV 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: 2461082.73532609 11.02.2026 05:38:42.174 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
First image: 2461082.73532609 11.02.2026 05:38:42.174 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Last image: 2461186.62916101 26.05.2026 03:05:49.511 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.78
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 14798
Objects passed selection criteria: 14739
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: 9767.75
Average stars matched: 9131.75 (93.4888 %)
Memory usage VmPeak: 120140 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 22:10:12 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: 2461082.73532609 11.02.2026 05:38:42.174 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
First image: 2461082.73532609 11.02.2026 05:38:42.174 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Last image: 2461186.62916101 26.05.2026 03:05:49.511 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 79
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.44
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 14 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 88463
Objects passed selection criteria: 88270
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: 59792.2
Average stars matched: 58141.5 (97.2392 %)
Memory usage VmPeak: 2055944 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 22:12:21 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/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
SExtractor catalog cache: saved Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat to cache
SExtractor catalog cache: saved Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.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/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.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: 2461186.62863722
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits exists and is non-empty
Saving wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits to local_wcs_cache/
'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits' -> 'local_wcs_cache/wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits'
wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits exists and is non-empty
Saving wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits to local_wcs_cache/
'wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits' -> 'local_wcs_cache/wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits'
wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits exists and is non-empty
Saving wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits to local_wcs_cache/
'wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits' -> 'local_wcs_cache/wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits'
wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits exists and is non-empty
Saving wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits to local_wcs_cache/
'wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits' -> 'local_wcs_cache/wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits (1st reference image)
verification OK: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:17.999 -01:59:50.01 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits (1st new image)
verification OK: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.5'x626.7' 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: 08:34:21.379 -02:01:27.01 J2000 4789.000 3195.000
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###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:17.999 -01:59:50.01
Second-epoch image center 08:34:21.379 -02:01:27.01
Angular distance between the image centers 0.0304 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits (2nd new image)
verification OK: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
Image size: 941.5'x626.7' 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: 08:34:23.006 -02:00:48.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:34:17.999 -01:59:50.01
Second-epoch image center 08:34:23.006 -02:00:48.41
Angular distance between the image centers 0.0264 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 08:34:21.379 -02:01:27.01
Second-epoch second image center 08:34:23.006 -02:00:48.41
Angular distance between the image centers 0.01268 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/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits &> /tmp/tmp.RiVzWlmTnA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits &> /tmp/tmp.ntGe67HHIv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits &> /tmp/tmp.AwyFT1ZOPT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits &> /tmp/tmp.GXDyuy2dth
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.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_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.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_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
Found non-empty wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
The reference image (wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits) and catalog (wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat) found
'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat' -> 'wcsmag.cat'
Read 15397 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6688 to 136.5116 deg, Dec -7.3043 to +3.3173 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 120.6688 to 136.5116 deg, Dec -7.3043 to 3.3173 deg
Loaded 10194 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): 8099 out of 8827 total matches.
Matched with Tycho-2 8827 out of 15397 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.877700
a=0.000000 b=1.000000 c=22.877700
From vast_summary.log: estimated ref. image limiting mag.: -7.78
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 15397 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6688 to 136.5116 deg, Dec -7.3043 to +3.3173 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 120.6688 to 136.5116 deg, Dec -7.3043 to 3.3173 deg
Loaded 10194 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): 8099 out of 8827 total matches.
Matched with Tycho-2 8827 out of 15397 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits:
Forced-photometry filter: calibrated wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits (aperture=6.4)
Read 17191 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6917 to 136.5012 deg, Dec -7.2983 to +3.3042 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 120.6917 to 136.5012 deg, Dec -7.2983 to 3.3042 deg
Loaded 10153 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): 8425 out of 8877 total matches.
Matched with Tycho-2 8877 out of 17191 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits:
Forced-photometry filter: calibrated wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits -> calib.txt_param_ref_wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
2.5 pix Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
3.2 pix fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
3.3 pix fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
2.2 pix wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
2.5 pix wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Limiting magnitude estimates:
15.1 mag. Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
15.1 mag. Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
13.1 mag. fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
13.1 mag. fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.6 (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.RiVzWlmTnA (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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits' -> 'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Checking if the catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS catalog name: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1476, passed=15397
Got 15397 stars (including 13898 good ones) from the SExtractor catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
util/solve_plate_with_UCAC5 got 15397 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 14967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 14964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 14965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits N_match=930 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.479 sigma_q2_arcsec=0.417 sigma_q3_arcsec=0.450 sigma_q4_arcsec=0.426 n_q1=263 n_q2=220 n_q3=237 n_q4=210 worst_quadrant_to_overall_ratio=1.042
The image catalog is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits -region wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.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.ntGe67HHIv (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/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits' -> 'wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS-calibrated image found: wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Checking if the catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS catalog name: wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1131, passed=17191
Got 17191 stars (including 16043 good ones) from the SExtractor catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat
util/solve_plate_with_UCAC5 got 17191 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 16766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 16766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 16766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits N_match=930 sigma_overall_arcsec=0.455 sigma_q1_arcsec=0.376 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.459 n_q1=179 n_q2=260 n_q3=197 n_q4=294 worst_quadrant_to_overall_ratio=1.274
The image catalog is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits -region wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.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.AwyFT1ZOPT (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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
Checking if the catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
WCS catalog name: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=190, passed=3435
Got 3435 stars (including 3242 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat
util/solve_plate_with_UCAC5 got 3435 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 411 to 469 (Dec -7.7 to 3.5)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 3262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 469 (Dec -7.7 to 3.5)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 3264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 3264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 919 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits N_match=919 sigma_overall_arcsec=0.449 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.508 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.641 n_q1=301 n_q2=175 n_q3=280 n_q4=163 worst_quadrant_to_overall_ratio=1.427
The image catalog is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits -region wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.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.GXDyuy2dth (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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
Checking if the catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
WCS catalog name: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=179, passed=3319
Got 3319 stars (including 3136 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat
util/solve_plate_with_UCAC5 got 3319 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 411 to 469 (Dec -7.7 to 3.5)
Done reading UCAC5 zone files...
Matched 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 3148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 469 (Dec -7.7 to 3.5)
Done reading UCAC5 zone files...
Matched 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 3147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 3147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits N_match=915 sigma_overall_arcsec=0.490 sigma_q1_arcsec=0.495 sigma_q2_arcsec=0.522 sigma_q3_arcsec=0.379 sigma_q4_arcsec=0.613 n_q1=294 n_q2=163 n_q3=275 n_q4=183 worst_quadrant_to_overall_ratio=1.252
The image catalog is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits -region wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.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=Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits sigma_overall=0.459 worst_q_ratio=1.042
ref2=Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits sigma_overall=0.455 worst_q_ratio=1.274
new1=fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits sigma_overall=0.449 worst_q_ratio=1.427
new2=fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits sigma_overall=0.490 worst_q_ratio=1.252
reference average sigma_overall=0.457 worst_q_ratio=1.158
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207_astrometric_residuals.png (930 matched stars from wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085_astrometric_residuals.png (930 matched stars from wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024_astrometric_residuals.png (919 matched stars from wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025_astrometric_residuals.png (915 matched stars from wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits'
Saving fully-calibrated image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits'
Preparing the HTML report for the field Hya-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Hya-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
SExtractor catalog cache: saved Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat to cache
SExtractor catalog cache: saved Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Creating symlink local_wcs_cache/wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.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_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits exists and is non-empty
wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits exists and is non-empty
wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits exists and is non-empty
wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits (1st reference image)
verification OK: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:17.999 -01:59:50.01 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits (1st new image)
verification OK: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.5'x626.7' 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: 08:34:21.379 -02:01:27.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:17.999 -01:59:50.01
Second-epoch image center 08:34:21.379 -02:01:27.01
Angular distance between the image centers 0.0304 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits (2nd new image)
verification OK: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
Image size: 941.5'x626.7' 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: 08:34:23.006 -02:00:48.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:34:17.999 -01:59:50.01
Second-epoch image center 08:34:23.006 -02:00:48.41
Angular distance between the image centers 0.0264 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 08:34:21.379 -02:01:27.01
Second-epoch second image center 08:34:23.006 -02:00:48.41
Angular distance between the image centers 0.01268 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/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits &> /tmp/tmp.XVfgJmJOcY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits &> /tmp/tmp.gMVzH0VBvK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits &> /tmp/tmp.h2joWZ4Emz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits &> /tmp/tmp.zsk0b9sGUD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.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_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.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_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
Found non-empty wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
The reference image (wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits) and catalog (wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat) found
'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat' -> 'wcsmag.cat'
Read 104097 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6664 to 136.5280 deg, Dec -7.3049 to +3.3189 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 120.6664 to 136.5280 deg, Dec -7.3049 to 3.3189 deg
Loaded 10204 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): 7147 out of 9101 total matches.
Matched with Tycho-2 9101 out of 104097 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.721500
a=0.000000 b=1.000000 c=22.721500
From vast_summary.log: estimated ref. image limiting mag.: -7.44
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 104097 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6664 to 136.5280 deg, Dec -7.3049 to +3.3189 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 120.6664 to 136.5280 deg, Dec -7.3049 to 3.3189 deg
Loaded 10204 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): 7147 out of 9101 total matches.
Matched with Tycho-2 9101 out of 104097 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits:
Forced-photometry filter: calibrated wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits (aperture=4.7)
Read 94372 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6830 to 136.5033 deg, Dec -7.2984 to +3.3115 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 120.6830 to 136.5033 deg, Dec -7.2984 to 3.3115 deg
Loaded 10170 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): 7417 out of 8998 total matches.
Matched with Tycho-2 8998 out of 94372 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits:
Forced-photometry filter: calibrated wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits -> calib.txt_param_ref_wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits (aperture=5.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
2.4 pix Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
3.0 pix fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
3.0 pix fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
2.0 pix wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
2.4 pix wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Limiting magnitude estimates:
15.3 mag. Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
15.2 mag. Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
13.3 mag. fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
13.3 mag. fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 12.8 (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.XVfgJmJOcY (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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits' -> 'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Checking if the catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS catalog name: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=9087, passed=104070
Got 104070 stars (including 94791 good ones) from the SExtractor catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
util/solve_plate_with_UCAC5 got 104070 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 102214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 102208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 102209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits N_match=931 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.488 sigma_q2_arcsec=0.434 sigma_q3_arcsec=0.455 sigma_q4_arcsec=0.446 n_q1=264 n_q2=221 n_q3=243 n_q4=203 worst_quadrant_to_overall_ratio=1.063
The image catalog is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits -region wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.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.gMVzH0VBvK (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/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits' -> 'wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS-calibrated image found: wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Checking if the catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS catalog name: wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=8013, passed=94354
Got 94354 stars (including 86210 good ones) from the SExtractor catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat
util/solve_plate_with_UCAC5 got 94354 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 91878 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 413 to 468 (Dec -7.3 to 3.3)
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: 929 matched stars entering correct_measured_positions(), 91878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 91876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits N_match=929 sigma_overall_arcsec=0.450 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.562 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.488 n_q1=180 n_q2=271 n_q3=179 n_q4=299 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits -region wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.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.h2joWZ4Emz (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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
Checking if the catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
WCS catalog name: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=551, passed=21502
Got 21502 stars (including 20931 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat
util/solve_plate_with_UCAC5 got 21502 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 411 to 470 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 20343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 411 to 470 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 20339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 20339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 917 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits N_match=917 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.471 sigma_q2_arcsec=0.478 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.624 n_q1=305 n_q2=174 n_q3=279 n_q4=159 worst_quadrant_to_overall_ratio=1.407
The image catalog is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits -region wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.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.zsk0b9sGUD (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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
Checking if the catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
WCS catalog name: wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=524, passed=21050
Got 21050 stars (including 20496 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat
util/solve_plate_with_UCAC5 got 21050 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 411 to 470 (Dec -7.7 to 3.7)
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(), 877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 19877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 914 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(), 19874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 19874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits N_match=912 sigma_overall_arcsec=0.460 sigma_q1_arcsec=0.485 sigma_q2_arcsec=0.532 sigma_q3_arcsec=0.364 sigma_q4_arcsec=0.589 n_q1=299 n_q2=160 n_q3=274 n_q4=179 worst_quadrant_to_overall_ratio=1.283
The image catalog is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits -region wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.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_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-04_20.00sec_-0.00C_LIGHTs_0024.fits
Saving fully-calibrated image wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.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_Hya-03-Q1b1x1_220629_TTUQ1b1x1_896592_ERRakziW/wcs_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025.fits
Preparing the HTML report for the field Hya-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:46:41.26 -00:20:36.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:08:05.88 -00:02:44.7: 10.56 +/- 0.00 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:46:30.71 +02:51:34.1: 13.21 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 09:01:28.54 -04:28:30.4: 12.67 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:36.22 -05:09:49.5: 12.29 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:46:41.26 -00:20:36.6: 12.59 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:08:05.88 -00:02:44.7: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:46:30.71 +02:51:34.1: 13.11 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 08:46:41.26 -00:20:36.6: ref_mag=12.63 +/- 0.01 new_mean_mag=12.5080 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 10.55 +/- 0.00
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter REJECTED candidate at 08:08:05.88 -00:02:44.7: ref_mag=10.55 +/- 0.00 new_mean_mag=11.8590 delta=-1.31 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 09:01:28.54 -04:28:30.4: 12.51 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 08:46:30.71 +02:51:34.1: ref_mag=13.16 +/- 0.02 new_mean_mag=12.7687 delta=0.39 (need > 0.90)
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Forced photometry filter REJECTED candidate at 09:01:28.54 -04:28:30.4: ref_mag=12.57 +/- 0.02 new_mean_mag=12.5348 delta=0.04 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:17.44 -05:47:55.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:08.09 -05:31:38.5: 12.06 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:48.10 -06:05:55.6: 12.65 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:58.52 -04:57:18.2: 12.32 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:56.44 -06:34:04.1: 12.60 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:36.22 -05:09:49.5: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 08:03:36.22 -05:09:49.5: ref_mag=12.32 +/- 0.01 new_mean_mag=11.3779 delta=0.94 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:08.09 -05:31:38.5: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:48.10 -06:05:55.6: 12.65 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 08:04:08.09 -05:31:38.5: ref_mag=12.07 +/- 0.01 new_mean_mag=11.1771 delta=0.90 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:17.44 -05:47:55.0: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter KEPT candidate at 08:03:48.10 -06:05:55.6: ref_mag=12.65 +/- 0.02 new_mean_mag=11.6807 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter KEPT candidate at 08:04:17.44 -05:47:55.0: ref_mag=12.65 +/- 0.02 new_mean_mag=11.6325 delta=1.01 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:58.52 -04:57:18.2: 12.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 08:03:58.52 -04:57:18.2: ref_mag=12.34 +/- 0.01 new_mean_mag=11.4105 delta=0.93 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:56.44 -06:34:04.1: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry filter KEPT candidate at 08:04:56.44 -06:34:04.1: ref_mag=12.62 +/- 0.02 new_mean_mag=11.5647 delta=1.06 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:22.23 -06:18:43.2: 12.56 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:07:31.79 -06:37:09.2: 12.56 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:07:48.71 -05:03:21.9: 11.79 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:05:31.23 -06:01:48.6: 12.29 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:07:31.79 -06:37:09.2: 12.47 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:07:48.71 -05:03:21.9: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:05:31.23 -06:01:48.6: 11.76 +/- 0.01 detection
Forced photometry filter KEPT candidate at 08:07:31.79 -06:37:09.2: ref_mag=12.51 +/- 0.02 new_mean_mag=11.5807 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Forced photometry filter KEPT candidate at 08:05:31.23 -06:01:48.6: ref_mag=11.92 +/- 0.01 new_mean_mag=10.9562 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 08:07:48.71 -05:03:21.9: ref_mag=11.50 +/- 0.01 new_mean_mag=10.5600 delta=0.94 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:22.23 -06:18:43.2: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry filter KEPT candidate at 08:04:22.23 -06:18:43.2: ref_mag=12.56 +/- 0.02 new_mean_mag=11.5627 delta=1.00 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:41.13 -06:31:46.4: 12.54 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:41.13 -06:31:46.4: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Forced photometry filter KEPT candidate at 08:04:41.13 -06:31:46.4: ref_mag=12.55 +/- 0.02 new_mean_mag=11.6176 delta=0.93 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:20.80 -05:59:02.0: 12.94 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:20.80 -05:59:02.0: 12.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter KEPT candidate at 08:04:20.80 -05:59:02.0: ref_mag=12.93 +/- 0.02 new_mean_mag=11.9325 delta=1.00 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:05:21.27 -05:46:38.9: 12.16 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:36.32 -06:18:15.5: 12.17 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:06:18.26 -06:11:57.4: 12.90 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:05:21.27 -05:46:38.9: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter KEPT candidate at 08:05:21.27 -05:46:38.9: ref_mag=12.17 +/- 0.01 new_mean_mag=11.2444 delta=0.93 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:06:04.66 -06:34:40.3: 12.47 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:36.32 -06:18:15.5: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 08:03:36.32 -06:18:15.5: ref_mag=12.18 +/- 0.01 new_mean_mag=11.1442 delta=1.04 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:06:18.26 -06:11:57.4: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 08:06:18.26 -06:11:57.4: ref_mag=12.92 +/- 0.02 new_mean_mag=11.9159 delta=1.01 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:06:04.66 -06:34:40.3: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter KEPT candidate at 08:06:04.66 -06:34:40.3: ref_mag=12.44 +/- 0.01 new_mean_mag=11.4926 delta=0.95 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:35.79 -06:21:59.1: 12.11 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:35.79 -06:21:59.1: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 08:03:35.79 -06:21:59.1: ref_mag=12.12 +/- 0.01 new_mean_mag=11.1870 delta=0.94 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:37.04 -06:03:02.5: 12.88 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:53.96 -06:16:21.4: 12.86 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:37.04 -06:03:02.5: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter KEPT candidate at 08:04:37.04 -06:03:02.5: ref_mag=12.90 +/- 0.02 new_mean_mag=11.8628 delta=1.03 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:53.96 -06:16:21.4: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter KEPT candidate at 08:03:53.96 -06:16:21.4: ref_mag=12.88 +/- 0.02 new_mean_mag=11.8739 delta=1.00 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:05:17.75 -06:22:33.1: 12.13 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:05:17.75 -06:22:33.1: 12.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter KEPT candidate at 08:05:17.75 -06:22:33.1: ref_mag=12.14 +/- 0.01 new_mean_mag=11.1941 delta=0.94 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:57.94 -05:16:46.9: 12.86 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:57.94 -05:16:46.9: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry filter KEPT candidate at 08:03:57.94 -05:16:46.9: ref_mag=12.86 +/- 0.02 new_mean_mag=11.8831 delta=0.98 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:04.06 -05:26:25.2: 12.85 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:04.06 -05:26:25.2: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter KEPT candidate at 08:04:04.06 -05:26:25.2: ref_mag=12.88 +/- 0.02 new_mean_mag=11.8258 delta=1.05 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:54:51.58 +01:05:26.4: 13.42 +/- 0.04 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:54:51.58 +01:05:26.4: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter REJECTED candidate at 08:54:51.58 +01:05:26.4: ref_mag=13.42 +/- 0.03 new_mean_mag=12.8690 delta=0.55 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:05:18.89 -06:32:33.5: 13.11 +/- 0.04 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:05:18.89 -06:32:33.5: 13.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter KEPT candidate at 08:05:18.89 -06:32:33.5: ref_mag=13.08 +/- 0.03 new_mean_mag=11.8880 delta=1.19 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:09.43 -06:24:29.9: 11.99 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:09.43 -06:24:29.9: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter KEPT candidate at 08:04:09.43 -06:24:29.9: ref_mag=11.99 +/- 0.01 new_mean_mag=11.0246 delta=0.97 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:05:40.58 -05:53:11.3: 12.40 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:03:29.68 -05:24:44.6: 12.39 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:21.16 -05:50:08.4: 12.37 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:05:40.58 -05:53:11.3: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter REJECTED candidate at 08:05:40.58 -05:53:11.3: ref_mag=12.40 +/- 0.01 new_mean_mag=11.4987 delta=0.90 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:03:29.68 -05:24:44.6: 12.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 08:03:29.68 -05:24:44.6: ref_mag=12.35 +/- 0.01 new_mean_mag=11.3679 delta=0.98 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:21.16 -05:50:08.4: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 08:04:21.16 -05:50:08.4: ref_mag=12.35 +/- 0.01 new_mean_mag=11.4282 delta=0.92 (need > 0.90)
Adding exclusion_list_local.txt__out06721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23880.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 34s
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: 12s
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Considering the candidate 120002_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120002_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
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Considering the candidate 120252_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120252_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 09:05:13.53 +02:23:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120309_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120309_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 08:46:15.95 +01:35:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120346_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120346_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
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Considering the candidate 120387_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120387_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 08:31:20.91 -06:39:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120397_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120397_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 08:26:27.83 -03:57:58.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 120406_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120406_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
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Considering the candidate 120439_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120439_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 08:55:10.77 +02:36:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120461_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120461_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
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Considering the candidate 120464_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120464_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 08:35:46.32 -00:25:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120545_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120545_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 08:44:45.06 +01:42:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120569_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 120569_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 08:50:20.62 -04:10:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21874_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 21874_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 17676_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 17676_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
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Considering the candidate 11958_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 11958_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 15179_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 15179_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 23880_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 23880_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 07200_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 07200_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 22675_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 22675_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 12487_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 12487_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 09815_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 09815_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 06721_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 06721_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 07604_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 07604_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 13217_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 13217_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 100254_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 100254_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 09:02:41.33 -00:13:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15350_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 15350_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 09846_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 09846_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 11029_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 11029_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 07097_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 07097_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 09135_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 09135_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 12470_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 12470_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
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Considering the candidate 10216_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 10216_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09117_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 09117_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20596_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 20596_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18931_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 18931_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87708_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 87708_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07458_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 07458_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08666_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 08666_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08029_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 08029_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
**** FOUND 08:03:52.05 -06:28:53.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14234_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
The candidate 14234_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19141_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 19141_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14725_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
Preparing report for the candidate 14725_fd_Hya-03-Q1b1x1_2026-05-25_22-05-49_20.00sec_-0.00C_LIGHTs_0025
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 47s
Prepared the HTML report for the field Hya-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:07:31.79 -06:37:09.2
08:06:04.66 -06:34:40.3
08:04:56.44 -06:34:04.1
08:05:18.89 -06:32:33.5
08:04:41.13 -06:31:46.4
08:04:09.43 -06:24:29.9
08:05:17.75 -06:22:33.1
08:03:35.79 -06:21:59.1
08:04:22.23 -06:18:43.2
08:03:36.32 -06:18:15.5
08:03:53.96 -06:16:21.4
08:06:18.26 -06:11:57.4
08:03:48.10 -06:05:55.6
08:04:37.04 -06:03:02.5
08:05:31.23 -06:01:48.6
08:04:20.80 -05:59:02.0
08:04:21.16 -05:50:08.4
08:04:17.44 -05:47:55.0
08:05:21.27 -05:46:38.9
08:04:04.06 -05:26:25.2
08:03:29.68 -05:24:44.6
08:03:57.94 -05:16:46.9
08:03:36.22 -05:09:49.5
08:07:48.71 -05:03:21.9
08:03:58.52 -04:57:18.2
########### Completed Hya-03-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 ####
08:03:36.22 -05:09:49.5
08:03:48.10 -06:05:55.6
08:04:17.44 -05:47:55.0
08:03:58.52 -04:57:18.2
08:04:56.44 -06:34:04.1
08:07:48.71 -05:03:21.9
08:05:31.23 -06:01:48.6
08:04:22.23 -06:18:43.2
08:07:31.79 -06:37:09.2
08:04:41.13 -06:31:46.4
08:04:20.80 -05:59:02.0
08:05:21.27 -05:46:38.9
08:03:36.32 -06:18:15.5
08:06:18.26 -06:11:57.4
08:06:04.66 -06:34:40.3
08:03:35.79 -06:21:59.1
08:04:37.04 -06:03:02.5
08:03:53.96 -06:16:21.4
08:05:17.75 -06:22:33.1
08:03:57.94 -05:16:46.9
08:04:04.06 -05:26:25.2
08:05:18.89 -06:32:33.5
08:04:09.43 -06:24:29.9
08:03:29.68 -05:24:44.6
08:04:21.16 -05:50:08.4
###################################################################################
08:03:36.22 -05:09:49.5 -- not an asteroid (will add it to exclusion list)
08:03:48.10 -06:05:55.6 -- not an asteroid (will add it to exclusion list)
08:04:17.44 -05:47:55.0 -- not an asteroid (will add it to exclusion list)
08:03:58.52 -04:57:18.2 -- not an asteroid (will add it to exclusion list)
08:04:56.44 -06:34:04.1 -- not an asteroid (will add it to exclusion list)
08:07:48.71 -05:03:21.9 -- not an asteroid (will add it to exclusion list)
08:05:31.23 -06:01:48.6 -- not an asteroid (will add it to exclusion list)
08:04:22.23 -06:18:43.2 -- not an asteroid (will add it to exclusion list)
08:07:31.79 -06:37:09.2 -- not an asteroid (will add it to exclusion list)
08:04:41.13 -06:31:46.4 -- not an asteroid (will add it to exclusion list)
08:04:20.80 -05:59:02.0 -- not an asteroid (will add it to exclusion list)
08:05:21.27 -05:46:38.9 -- not an asteroid (will add it to exclusion list)
08:03:36.32 -06:18:15.5 -- not an asteroid (will add it to exclusion list)
08:06:18.26 -06:11:57.4 -- not an asteroid (will add it to exclusion list)
08:06:04.66 -06:34:40.3 -- not an asteroid (will add it to exclusion list)
08:03:35.79 -06:21:59.1 -- not an asteroid (will add it to exclusion list)
08:04:37.04 -06:03:02.5 -- not an asteroid (will add it to exclusion list)
08:03:53.96 -06:16:21.4 -- not an asteroid (will add it to exclusion list)
08:05:17.75 -06:22:33.1 -- not an asteroid (will add it to exclusion list)
08:03:57.94 -05:16:46.9 -- not an asteroid (will add it to exclusion list)
08:04:04.06 -05:26:25.2 -- not an asteroid (will add it to exclusion list)
08:05:18.89 -06:32:33.5 -- not an asteroid (will add it to exclusion list)
08:04:09.43 -06:24:29.9 -- not an asteroid (will add it to exclusion list)
08:03:29.68 -05:24:44.6 -- not an asteroid (will add it to exclusion list)
08:04:21.16 -05:50:08.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
08:03:29.68 -05:24:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:03:35.79 -06:21:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:03:36.22 -05:09:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:03:36.32 -06:18:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:03:48.10 -06:05:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:03:53.96 -06:16:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:03:57.94 -05:16:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:03:58.52 -04:57:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:04.06 -05:26:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:09.43 -06:24:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:17.44 -05:47:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:20.80 -05:59:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:21.16 -05:50:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:22.23 -06:18:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:37.04 -06:03:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:41.13 -06:31:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:56.44 -06:34:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:05:17.75 -06:22:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:05:18.89 -06:32:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:05:21.27 -05:46:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:05:31.23 -06:01:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:06:04.66 -06:34:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:06:18.26 -06:11:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:07:31.79 -06:37:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:07:48.71 -05:03:21.9 -- 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)
08:03:29.68 -05:24:44.6 -- not a known variable star
08:03:35.79 -06:21:59.1 -- not a known variable star
08:03:36.22 -05:09:49.5 -- a known variable star
08:03:36.32 -06:18:15.5 -- not a known variable star
08:03:48.10 -06:05:55.6 -- a known variable star
08:03:53.96 -06:16:21.4 -- not a known variable star
08:03:57.94 -05:16:46.9 -- not a known variable star
08:03:58.52 -04:57:18.2 -- a known variable star
08:04:04.06 -05:26:25.2 -- not a known variable star
08:04:09.43 -06:24:29.9 -- not a known variable star
08:04:17.44 -05:47:55.0 -- not a known variable star
08:04:20.80 -05:59:02.0 -- not a known variable star
08:04:21.16 -05:50:08.4 -- not a known variable star
08:04:22.23 -06:18:43.2 -- a known variable star
08:04:37.04 -06:03:02.5 -- a known variable star
08:04:41.13 -06:31:46.4 -- not a known variable star
08:04:56.44 -06:34:04.1 -- not a known variable star
08:05:17.75 -06:22:33.1 -- not a known variable star
08:05:18.89 -06:32:33.5 -- not a known variable star
08:05:21.27 -05:46:38.9 -- not a known variable star
08:05:31.23 -06:01:48.6 -- a known variable star
08:06:04.66 -06:34:40.3 -- not a known variable star
08:06:18.26 -06:11:57.4 -- not a known variable star
08:07:31.79 -06:37:09.2 -- not a known variable star
08:07:48.71 -05:03:21.9 -- a known variable star
Found 18 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
25 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
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 ####
08:03:29.68 -05:24:44.6
08:03:35.79 -06:21:59.1
08:03:36.22 -05:09:49.5
08:03:36.32 -06:18:15.5
08:03:48.10 -06:05:55.6
08:03:53.96 -06:16:21.4
08:03:57.94 -05:16:46.9
08:03:58.52 -04:57:18.2
08:04:04.06 -05:26:25.2
08:04:09.43 -06:24:29.9
08:04:17.44 -05:47:55.0
08:04:20.80 -05:59:02.0
08:04:21.16 -05:50:08.4
08:04:22.23 -06:18:43.2
08:04:37.04 -06:03:02.5
08:04:41.13 -06:31:46.4
08:04:56.44 -06:34:04.1
08:05:17.75 -06:22:33.1
08:05:18.89 -06:32:33.5
08:05:21.27 -05:46:38.9
08:05:31.23 -06:01:48.6
08:06:04.66 -06:34:40.3
08:06:18.26 -06:11:57.4
08:07:31.79 -06:37:09.2
08:07:48.71 -05:03:21.9
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461186.62863722 -observatory V36
05:06:44.01 +24:42:20.4 Mercury (-1.1mag)
06:35:37.01 +24:59:10.5 Venus (-3.9mag)
02:11:53.64 +12:33:01.4 Mars (1.3mag)
07:37:56.61 +21:56:31.7 Jupiter (-1.9mag)
00:45:16.89 +02:25:46.5 Saturn (0.9mag)
03:57:03.34 +20:16:16.5 Uranus (5.8mag)
00:15:13.44 +00:11:32.1 Neptune (7.8mag)
20:33:56.37 -23:00:02.8 Pluto (14.5mag)
12:18:23.25 -05:27:41.9 Moon (-11.2mag)
-rw-r--r-- 1 apache apache 363 May 25 22:10 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461186.62863722:
07:37:52.72 +21:56:40.9 Io (5.9mag)
07:38:07.70 +21:56:00.3 Europa (6.1mag)
07:37:48.67 +21:56:58.5 Ganymede (5.5mag)
07:37:35.32 +21:57:23.5 Callisto (6.7mag)
07:39:01.92 +21:32:52.5 Himalia (15.5mag)
07:37:55.11 +21:56:37.4 Thebe (16.5mag)
07:39:20.34 +21:54:09.4 Elara (17.5mag)
07:39:24.20 +22:15:18.7 Pasiphae (17.7mag)
07:45:03.85 +21:57:21.0 Carme (18.8mag)
00:45:18.77 +02:25:27.0 Titan (8.7mag)
00:45:12.87 +02:25:55.3 Rhea (10.0mag)
00:45:39.47 +02:25:52.7 Iapetus (11.4mag)
00:45:31.71 +02:25:48.9 Hyperion (14.7mag)
00:46:14.60 +02:29:33.9 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 25 22:10 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461186.62863722:
17:17:29.79 -33:17:45.2 JWST
15:53:13.04 +52:55:55.4 Chandra
08:06:16.30 -41:22:09.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 25 22:10 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461186.62863722 -observatory V36
13:20:49.86 -27:03:57.2 14.4mag D/1884 O1 (Barnard)
06:37:16.59 +30:40:24.9 15.7mag D/1886 K1 (Brooks)
15:26:20.78 +01:20:49.8 14.6mag D/1895 Q1 (Swift)
05:28:05.48 +24:38:47.9 17.2mag D/1918 W1 (Schorr)
09:30:59.65 +14:35:46.6 17.9mag P/2009 WX51 (Catalina)
18:51:02.55 -31:39:10.1 13.7mag P/2010 H2 (Vales)
05:40:49.94 -68:16:06.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:20.19 +31:48:27.9 17.4mag C/2017 K2 (PANSTARRS)
17:19:52.93 +14:32:42.2 17.7mag C/2021 G2 (ATLAS)
23:14:33.07 +31:02:40.6 17.2mag C/2022 E2 (ATLAS)
05:17:56.55 +26:51:26.3 16.4mag C/2022 N2 (PANSTARRS)
09:20:55.79 +31:29:41.8 16.5mag C/2022 QE78 (ATLAS)
08:43:59.61 +03:12:54.5 17.6mag C/2022 R6 (PANSTARRS)
18:36:23.63 +21:12:08.5 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:28.35 -11:02:17.4 17.5mag P/2023 B1 (PANSTARRS)
22:16:12.18 +65:39:31.5 17.7mag C/2023 H5 (Lemmon)
18:17:13.28 -05:31:54.1 13.7mag C/2023 R1 (PANSTARRS)
13:39:59.73 +85:48:40.9 17.9mag C/2023 X2 (Lemmon)
06:53:22.12 +63:55:38.0 17.6mag C/2024 A1 (ATLAS)
06:26:48.02 +26:28:30.9 13.1mag C/2024 E1 (Wierzchos)
15:47:55.70 +12:12:10.6 17.3mag C/2024 G6 (ATLAS)
20:19:49.13 +27:09:27.0 14.1mag C/2024 J3 (ATLAS)
04:04:55.71 -17:12:34.9 16.1mag C/2024 T5 (ATLAS)
05:53:36.54 +36:49:29.8 17.9mag C/2025 J1 (Borisov)
11:45:45.64 +53:20:18.5 16.9mag C/2025 L1 (ATLAS)
06:24:48.93 -10:11:04.6 12.6mag C/2025 R3 (PANSTARRS)
12:40:57.77 +04:36:56.3 17.2mag C/2025 Y1 (ATLAS)
01:36:12.50 +42:22:39.3 15.7mag C/2026 B2 (Sun-Gao)
11:10:26.86 -09:00:43.5 16.3mag A/2026 E1
19:59:34.15 -08:07:24.0 9.5mag 10P/Tempel
14:18:47.05 -02:34:51.5 17.6mag 24P/Schaumasse
10:59:42.81 -00:51:54.8 15.9mag 29P/Schwassmann-Wachmann
10:51:17.11 -02:34:27.8 17.8mag 43P/Wolf-Harrington
02:51:22.56 +23:49:42.3 17.6mag 47P/Ashbrook-Jackson
08:32:07.99 +27:22:58.0 16.9mag 63P/Wild
00:14:49.87 -07:19:35.8 15.7mag 65P/Gunn
06:01:28.40 +31:40:35.5 16.5mag 76P/West-Kohoutek-Ikemura
02:37:50.20 +15:22:56.1 13.9mag 78P/Gehrels
00:51:01.47 +01:48:23.5 15.3mag 88P/Howell
04:12:36.01 +28:56:15.6 15.1mag 93P/Lovas
02:07:16.46 +25:20:36.1 17.9mag 114P/Wiseman-Skiff
06:19:52.23 +33:19:29.8 15.7mag 123P/West-Hartley
09:27:52.15 +20:17:33.6 16.4mag 124P/Mrkos
03:37:30.89 +18:17:06.4 16.4mag 128P/Shoemaker-Holt
04:07:27.86 +18:20:41.3 17.7mag 131P/Mueller
04:58:26.57 +19:38:48.5 13.0mag 141P/Machholz
05:01:05.46 +16:22:27.5 12.9mag 141P-A/Machholz
03:46:14.00 +13:42:20.2 10.6mag 141P-D/Machholz
02:48:09.40 -26:39:44.2 17.3mag 161P/Hartley-IRAS
02:59:43.92 +18:12:30.6 14.9mag 162P/SidingSpring
19:34:43.85 -01:43:26.6 17.6mag 169P/NEAT
17:02:23.83 -09:21:48.6 16.2mag 235P/LINEAR
07:04:54.68 +35:51:56.3 17.3mag 240P/NEAT
23:58:24.86 -07:47:28.7 16.7mag 260P/McNaught
03:29:52.02 +29:54:41.9 17.7mag 295P/LINEAR
22:04:42.02 -27:34:25.2 17.7mag 320P/McNaught
15:21:46.53 +08:21:38.1 17.4mag 391P/Kowalski
07:57:10.85 +21:02:22.8 17.8mag 450P/LONEOS
06:38:40.26 +42:35:27.5 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 25 22:10 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 22:10 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 22:10 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 22:10 tns_transients_list.txt
