This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.40 04:00:25.77 -22:08:53.7
217.03894 -47.01038 galactic Eri Second-epoch detections are separated by 1.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:00:25.77 -22:08:53.7 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.034 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:25.77 -22:08:53.7: 13.52 +/- 0.06 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:25.77 -22:08:53.7: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 04 00 25.77 -22 08 53.7 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.40,0.05,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 20260917.4582 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 11.35 03:41:13.52 -25:30:51.8
220.38616 -52.10048 galactic For Second-epoch detections are separated by 0.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J055.3057-25.5173 | 03:41:13.51 -25:30:51.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.591+/-0.032 (K)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:41:13.52 -25:30:51.8: 12.32 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:41:13.52 -25:30:51.8: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 41 13.52 -25 30 51.8 11.3 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J055.3057-25.5173,2461300.9582,11.35,0.05,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 J055.3057-25.5173 20260917.4582 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.16 03:47:35.24 -23:44:30.9
218.16396 -50.28572 galactic Eri Second-epoch detections are separated by 0.6" and 2.5 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 | 03:47:35.24 -23:44:30.9 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.031 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:47:35.24 -23:44:30.9: 13.11 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:47:35.24 -23:44:30.9: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 47 35.24 -23 44 30.9 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.16,0.05,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 20260917.4582 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.12 03:59:39.50 -22:50:49.5
217.95332 -47.37649 galactic Eri Second-epoch detections are separated by 0.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:59:39.50 -22:50:49.5 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.036 (F)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:59:39.50 -22:50:49.5: 13.11 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:59:39.50 -22:50:49.5: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 59 39.50 -22 50 49.5 12.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.4582 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.17 04:01:57.18 -23:18:10.8
218.80858 -46.99110 galactic Eri Second-epoch detections are separated by 0.6" and 2.5 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 | 04:01:57.18 -23:18:10.8 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.040 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:01:57.18 -23:18:10.8: 13.06 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:01:57.18 -23:18:10.8: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 04 01 57.18 -23 18 10.8 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.17,0.05,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 20260917.4582 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.09 04:00:32.48 -22:45:04.2
217.89953 -47.15449 galactic Eri Second-epoch detections are separated by 0.2" and 2.6 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 | 04:00:32.48 -22:45:04.2 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.034 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:32.48 -22:45:04.2: 13.03 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:32.48 -22:45:04.2: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 04 00 32.48 -22 45 04.2 12.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.09,0.05,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 20260917.4582 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 11.96 04:00:21.59 -22:41:38.9
217.80194 -47.17902 galactic Eri Second-epoch detections are separated by 0.5" and 2.7 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 | target | 04:00:21.59 -22:41:38.9 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.044 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:21.59 -22:41:38.9: 12.92 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:21.59 -22:41:38.9: 12.91 +/- 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!
TCP 2026 09 17.4582* 04 00 21.59 -22 41 38.9 12.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,11.96,0.05,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
target 20260917.4582 11.96CV 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 09 17.4582 2461300.9582 11.85 04:09:43.78 -22:49:07.9
218.83933 -45.13808 galactic Eri Second-epoch detections are separated by 0.3" and 2.6 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 | 04:09:43.78 -22:49:07.9 (user input) | T | P | (position from user input) J-Ks=0.491+/-0.030 (K)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:09:43.78 -22:49:07.9: 12.91 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:09:43.78 -22:49:07.9: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 04 09 43.78 -22 49 07.9 11.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,11.85,0.05,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 20260917.4582 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 11.88 03:37:30.33 -23:20:08.1
216.60250 -52.41976 galactic Eri Second-epoch detections are separated by 1.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:37:30.33 -23:20:08.1 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.031 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:37:30.33 -23:20:08.1: 12.87 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:37:30.33 -23:20:08.1: 12.77 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 37 30.33 -23 20 08.1 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,11.88,0.05,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
target 20260917.4582 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 09 17.4582 2461300.9582 11.95 04:02:27.53 -23:20:43.7
218.91377 -46.89045 galactic Eri Second-epoch detections are separated by 0.4" and 2.6 pix
The object was found in VSX12" Gaia DR3 5089442001294116992
Type: RS
# Max. Min./Amp. JD0 Period
15.050 G 15.120 G K
ATTENTION: measured mag 11.95 is 3.1 mag brighter than the VSX record maximum brightness 15.05 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:02:27.53 -23:20:43.7: 12.87 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:02:27.53 -23:20:43.7: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 04 02 27.53 -23 20 43.7 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5089442001294116992,2461300.9582,11.95,0.05,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
Gaia DR3 5089442001294116992 20260917.4582 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 09 17.4582 2461300.9582 11.84 03:47:18.30 -23:43:23.2
218.11013 -50.34357 galactic Eri Second-epoch detections are separated by 0.3" and 2.6 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 | 03:47:18.30 -23:43:23.2 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.035 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:47:18.30 -23:43:23.2: 12.86 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:47:18.30 -23:43:23.2: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 47 18.30 -23 43 23.2 11.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,11.84,0.05,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 20260917.4582 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 11.64 03:49:43.52 -24:07:24.4
218.92836 -49.90652 galactic For Second-epoch detections are separated by 0.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5083933825996762496 | 03:49:43.53 -24:07:24.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.406+/-0.032 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:49:43.52 -24:07:24.4: 12.61 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:49:43.52 -24:07:24.4: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 49 43.52 -24 07 24.4 11.6 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5083933825996762496,2461300.9582,11.64,0.05,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 5083933825996762496 20260917.4582 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 11.60 03:40:29.21 -25:32:24.0
220.37026 -52.26875 galactic For Second-epoch detections are separated by 1.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5085163492313693184 | 03:40:29.25 -25:32:23.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.371+/-0.033 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:40:29.21 -25:32:24.0: 12.58 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:40:29.21 -25:32:24.0: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 40 29.21 -25 32 24.0 11.6 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5085163492313693184,2461300.9582,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5085163492313693184 20260917.4582 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 11.57 03:38:43.38 -25:16:35.7
219.81037 -52.60271 galactic For Second-epoch detections are separated by 0.3" and 2.5 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 5085209740521492736 | 03:38:43.35 -25:16:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.258+/-0.032 (F)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:38:43.38 -25:16:35.7: 12.56 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:38:43.38 -25:16:35.7: 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!
TCP 2026 09 17.4582* 03 38 43.38 -25 16 35.7 11.6 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5085209740521492736,2461300.9582,11.57,0.05,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 5085209740521492736 20260917.4582 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 11.52 03:40:29.43 -25:19:47.5
220.03503 -52.22370 galactic For Second-epoch detections are separated by 0.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5085182115291880448 | 03:40:29.45 -25:19:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.244+/-0.033 (F)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:40:29.43 -25:19:47.5: 12.48 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:40:29.43 -25:19:47.5: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 40 29.43 -25 19 47.5 11.5 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5085182115291880448,2461300.9582,11.52,0.05,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
Gaia DR3 5085182115291880448 20260917.4582 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 09 17.4582 2461300.9582 11.49 03:47:30.86 -23:37:04.0
217.96937 -50.27070 galactic Eri Second-epoch detections are separated by 0.7" and 2.5 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 5086977995736733312 | 03:47:30.86 -23:37:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.521+/-0.031 (K)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:47:30.86 -23:37:04.0: 12.43 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:47:30.86 -23:37:04.0: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 47 30.86 -23 37 04.0 11.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5086977995736733312,2461300.9582,11.49,0.05,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 5086977995736733312 20260917.4582 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 11.41 04:00:29.63 -22:59:14.9
218.22968 -47.22951 galactic Eri Second-epoch detections are separated by 0.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5090263851876283776 | 04:00:29.64 -22:59:14.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.241+/-0.037 (F)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:29.63 -22:59:14.9: 12.38 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:29.63 -22:59:14.9: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 04 00 29.63 -22 59 14.9 11.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5090263851876283776,2461300.9582,11.41,0.05,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 5090263851876283776 20260917.4582 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.33 03:40:41.66 -25:33:30.0
220.41546 -52.22679 galactic For Second-epoch detections are separated by 0.5" and 2.5 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 | 03:40:41.66 -25:33:30.0 (user input) | T | P | (position from user input) J-Ks=0.710+/-0.030 (K)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:40:41.66 -25:33:30.0: 13.56 +/- 0.06 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:40:41.66 -25:33:30.0: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 40 41.66 -25 33 30.0 12.3 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.33,0.05,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 20260917.4582 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.37 03:38:20.74 -23:29:32.8
216.93055 -52.27280 galactic Eri Second-epoch detections are separated by 0.4" and 2.6 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 | 03:38:20.74 -23:29:32.8 (user input) | T | P | (position from user input) J-Ks=0.634+/-0.031 (K)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:38:20.74 -23:29:32.8: 13.56 +/- 0.06 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:38:20.74 -23:29:32.8: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 38 20.74 -23 29 32.8 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.37,0.05,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
target 20260917.4582 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.32 04:01:56.06 -23:19:33.3
218.83930 -47.00132 galactic Eri Second-epoch detections are separated by 0.7" and 2.7 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 | target | 04:01:56.06 -23:19:33.3 (user input) | T | P | (position from user input) J-Ks=0.538+/-0.038 (K)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:01:56.06 -23:19:33.3: 13.48 +/- 0.06 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:01:56.06 -23:19:33.3: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 04 01 56.06 -23 19 33.3 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.32,0.05,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 20260917.4582 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.29 03:47:58.22 -23:36:36.0
217.99886 -50.16767 galactic Eri Second-epoch detections are separated by 0.4" and 2.7 pix
The object was found in VSX 4" Gaia DR3 5086971329947521408
Type: ROT
# Max. Min./Amp. JD0 Period
15.720 G 15.770 G 3.352650000000 K
ATTENTION: measured mag 12.29 is 3.4 mag brighter than the VSX record maximum brightness 15.72 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:47:58.22 -23:36:36.0: 13.44 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:47:58.22 -23:36:36.0: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 47 58.22 -23 36 36.0 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5086971329947521408,2461300.9582,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5086971329947521408 20260917.4582 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.19 03:40:02.17 -25:33:20.0
220.36058 -52.37142 galactic For Second-epoch detections are separated by 1.3" and 2.6 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 | 03:40:02.17 -25:33:20.0 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.035 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:40:02.17 -25:33:20.0: 13.39 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:40:02.17 -25:33:20.0: 13.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 40 02.17 -25 33 20.0 12.2 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.19,0.05,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 20260917.4582 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.37 03:49:49.00 -24:04:00.2
218.85090 -49.87245 galactic For Second-epoch detections are separated by 1.0" and 2.5 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 | 03:49:49.00 -24:04:00.2 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.035 (K)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:49:49.00 -24:04:00.2: 13.38 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:49:49.00 -24:04:00.2: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 49 49.00 -24 04 00.2 12.4 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.37,0.05,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
target 20260917.4582 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.41 03:37:44.31 -23:17:58.2
216.56759 -52.35885 galactic Eri Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:37:44.31 -23:17:58.2 (user input) | T | P | (position from user input) J-Ks=0.856+/-0.038 (M)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:37:44.31 -23:17:58.2: 13.25 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:37:44.31 -23:17:58.2: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 37 44.31 -23 17 58.2 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.41,0.05,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 20260917.4582 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.35 03:48:28.52 -23:34:51.2
218.00064 -50.04838 galactic Eri Second-epoch detections are separated by 1.4" and 2.6 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 | 03:48:28.52 -23:34:51.2 (user input) | T | P | (position from user input) J-Ks=0.460+/-0.033 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:48:28.52 -23:34:51.2: 13.27 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:48:28.52 -23:34:51.2: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 03 48 28.52 -23 34 51.2 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.35,0.05,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 20260917.4582 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.11 04:00:44.65 -22:58:13.0
218.22830 -47.16939 galactic Eri Second-epoch detections are separated by 0.9" and 2.6 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 | 04:00:44.65 -22:58:13.0 (user input) | T | P | (position from user input) J-Ks=0.632+/-0.037 (K)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:44.65 -22:58:13.0: 13.19 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:44.65 -22:58:13.0: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 04 00 44.65 -22 58 13.0 12.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.4582 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.4582 2461300.9582 12.04 04:09:55.61 -22:49:06.2
218.85662 -45.09431 galactic Eri Second-epoch detections are separated by 2.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:09:55.61 -22:49:06.2 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.037 (G)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:09:55.61 -22:49:06.2: 13.18 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:09:55.61 -22:49:06.2: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 17.4582* 04 09 55.61 -22 49 06.2 12.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.9582,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.4582 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.63068376 18.01.2026 03:08:01.077 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
First image: 2461058.63068376 18.01.2026 03:08:01.077 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Last image: 2461300.95848631 17.09.2026 11:00:03.217 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.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.: -7.95
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: 2 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 4700
Objects passed selection criteria: 4671
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 2637.75
Average stars matched: 2538.5 (96.2373 %)
Memory usage VmPeak: 231352 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 17 06:01:53 CDT 2026
Host name: tau
############################################################
ERROR: large change in astrometric-star counts between the two new images (q3: 20 -> 14, 30.000% > 20%; fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits vs fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits) - possible passing clouds or a bad plate solution; continuing processing
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.63068376 18.01.2026 03:08:01.077 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
First image: 2461058.63068376 18.01.2026 03:08:01.077 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Last image: 2461300.95848631 17.09.2026 11:00:03.217 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 51
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 27337
Objects passed selection criteria: 27247
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 16687
Average stars matched: 16024.8 (96.0313 %)
Memory usage VmPeak: 251700 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 17 06:02:40 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
SExtractor catalog cache: saved Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.cat to cache
SExtractor catalog cache: saved Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.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/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.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: 2461300.95800641
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits exists and is non-empty
wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits exists and is non-empty
wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits exists and is non-empty
wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits (1st reference image)
verification OK: wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Image size: 941.7'x627.6' 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: 03:50:26.444 -26:00:02.47 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_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits (1st new image)
verification OK: wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
Image size: 941.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:50:22.426 -26:00:03.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:50:26.444 -26:00:02.47
Second-epoch image center 03:50:22.426 -26:00:03.39
Angular distance between the image centers 0.0150 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits (2nd new image)
verification OK: wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Image size: 941.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:50:23.053 -26:00:16.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:50:26.444 -26:00:02.47
Second-epoch image center 03:50:23.053 -26:00:16.24
Angular distance between the image centers 0.0133 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 03:50:22.426 -26:00:03.39
Second-epoch second image center 03:50:23.053 -26:00:16.24
Angular distance between the image centers 0.00427 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits &> /tmp/tmp.cgo2zRyDU8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits &> /tmp/tmp.4ySgf1YEKL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits &> /tmp/tmp.VLhHJbRTqK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits &> /tmp/tmp.3DcWO64Lq0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.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_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits and wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits and wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
Found non-empty wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits and wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
The reference image (wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits) and catalog (wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat) found
'wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat' -> 'wcsmag.cat'
Read 4897 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 48.7166 to 66.8986 deg, Dec -31.3420 to -20.3306 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 48.7166 to 66.8986 deg, Dec -31.3420 to -20.3306 deg
Loaded 6072 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): 3914 out of 4044 total matches.
Matched with Tycho-2 4044 out of 4897 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.761550
a=0.000000 b=1.000000 c=22.761550
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.81
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.81
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 4897 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 48.7166 to 66.8986 deg, Dec -31.3420 to -20.3306 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 48.7166 to 66.8986 deg, Dec -31.3420 to -20.3306 deg
Loaded 6072 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): 3914 out of 4044 total matches.
Matched with Tycho-2 4044 out of 4897 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Forced-photometry filter: calibrated wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits -> calib.txt_param_ref_wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits (aperture=6.0)
Read 5118 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 48.7169 to 66.8977 deg, Dec -31.3419 to -20.3060 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 48.7169 to 66.8977 deg, Dec -31.3419 to -20.3060 deg
Loaded 6079 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): 4024 out of 4155 total matches.
Matched with Tycho-2 4155 out of 5118 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
Forced-photometry filter: calibrated wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits -> calib.txt_param_ref_wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits (aperture=5.9)
____ 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: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
2.1 pix Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
1.9 pix fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
1.9 pix fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Limiting magnitude estimates:
14.8 mag. Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
14.9 mag. Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
11.6 mag. fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
11.9 mag. fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 9.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.cgo2zRyDU8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits' -> 'wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
WCS-calibrated image found: wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Checking if the catalog wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat corresponding to the image wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat corresponding to the image wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
WCS catalog name: wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=402, bad_region=0, passed=4897
Got 4897 stars (including 4486 good ones) from the SExtractor catalog wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
util/solve_plate_with_UCAC5 got 4897 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4390 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4389 matched stars entering correct_measured_positions(), 4389 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4389 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4390 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4388 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4388 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4388 stars left (next iteration limit 4827)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits N_match=4388 sigma_overall_arcsec=0.288 sigma_q1_arcsec=0.336 sigma_q2_arcsec=0.296 sigma_q3_arcsec=0.253 sigma_q4_arcsec=0.264 n_q1=1084 n_q2=1046 n_q3=1153 n_q4=1105 worst_quadrant_to_overall_ratio=1.169
The image catalog is written to wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits -region wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.4ySgf1YEKL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits' -> 'wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
WCS-calibrated image found: wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
Checking if the catalog wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
WCS catalog name: wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=394, bad_region=0, passed=5118
Got 5118 stars (including 4718 good ones) from the SExtractor catalog wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat
util/solve_plate_with_UCAC5 got 5118 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4610 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 4608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 5118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4610 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 5118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 5118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4607 stars left (next iteration limit 5067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits N_match=4607 sigma_overall_arcsec=0.276 sigma_q1_arcsec=0.331 sigma_q2_arcsec=0.278 sigma_q3_arcsec=0.257 sigma_q4_arcsec=0.246 n_q1=1122 n_q2=1085 n_q3=1235 n_q4=1165 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits -region wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.VLhHJbRTqK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
WCS_IMAGE_NAME=wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
WCS-calibrated image found: wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
Checking if the catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat corresponding to the image wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat corresponding to the image wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
WCS catalog name: wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=33, bad_region=0, passed=299
Got 299 stars (including 266 good ones) from the SExtractor catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat
util/solve_plate_with_UCAC5 got 299 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 294 to 350 (Dec -31.1 to -20.3)
Done reading UCAC5 zone files...
Matched 258 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 257 matched stars entering correct_measured_positions(), 150 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 257 matched stars entering correct_measured_positions(), 175 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 294 to 350 (Dec -31.1 to -20.3)
Done reading UCAC5 zone files...
Matched 258 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 257 matched stars entering correct_measured_positions(), 168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 257 matched stars entering correct_measured_positions(), 168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 257 stars left (next iteration limit 282)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=257 robust_rms=7.834 arcsec worst_quadrant_rms=21.669 arcsec
SIP_REFIT: SIP order 3 trial: matched=257 robust_rms=0.457 arcsec worst_quadrant_rms=0.529 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=257 robust_rms_before=0.823 arcsec robust_rms_before_corrected=0.465 arcsec robust_rms_after=0.457 arcsec worst_quadrant_rms_before=0.580 worst_quadrant_rms_after=0.529
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.580 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits N_match=257 sigma_overall_arcsec=0.429 sigma_q1_arcsec=0.422 sigma_q2_arcsec=0.479 sigma_q3_arcsec=0.372 sigma_q4_arcsec=0.393 n_q1=114 n_q2=84 n_q3=20 n_q4=39 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits -region wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.3DcWO64Lq0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
WCS_IMAGE_NAME=wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
WCS-calibrated image found: wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Checking if the catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat corresponding to the image wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat corresponding to the image wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
WCS catalog name: wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=25, bad_region=0, passed=298
Got 298 stars (including 273 good ones) from the SExtractor catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat
util/solve_plate_with_UCAC5 got 298 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 294 to 350 (Dec -31.1 to -20.3)
Done reading UCAC5 zone files...
Matched 261 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 260 matched stars entering correct_measured_positions(), 181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 260 matched stars entering correct_measured_positions(), 207 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 294 to 350 (Dec -31.1 to -20.3)
Done reading UCAC5 zone files...
Matched 261 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 260 matched stars entering correct_measured_positions(), 206 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 260 matched stars entering correct_measured_positions(), 206 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 260 stars left (next iteration limit 286)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 260 catalog matches do not cover the frame (119/89/14/38 per quadrant, need 16 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits N_match=260 sigma_overall_arcsec=0.543 sigma_q1_arcsec=0.461 sigma_q2_arcsec=0.479 sigma_q3_arcsec=0.655 sigma_q4_arcsec=0.482 n_q1=119 n_q2=89 n_q3=14 n_q4=38 worst_quadrant_to_overall_ratio=1.206
The image catalog is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits -region wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits to local_wcs_cache/
'wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits' -> 'local_wcs_cache/wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits'
Saving the final (post-refit) wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits to local_wcs_cache/
'wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits' -> 'local_wcs_cache/wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits'
Saving the final (post-refit) wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits to local_wcs_cache/
'wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits' -> 'local_wcs_cache/wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits'
Saving the final (post-refit) wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits to local_wcs_cache/
'wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits' -> 'local_wcs_cache/wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits sigma_overall=0.288 worst_q_ratio=1.169
ref2=Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits sigma_overall=0.276 worst_q_ratio=1.197
new1=fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits sigma_overall=0.429 worst_q_ratio=1.118
new2=fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits sigma_overall=0.543 worst_q_ratio=1.206
reference average sigma_overall=0.282 worst_q_ratio=1.183
warn-on-ratio threshold: 2.0x reference
###################################
ERROR: large change in astrometric-star counts between the two new images (q3: 20 -> 14, 30.000% > 20%; fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits vs fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits) - possible passing clouds or a bad plate solution; continuing processing
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076_astrometric_residuals.png (4388 matched stars from wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083_astrometric_residuals.png (4607 matched stars from wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101_astrometric_residuals.png (257 matched stars from wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102_astrometric_residuals.png (260 matched stars from wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits'
Saving fully-calibrated image wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits'
Preparing the HTML report for the field Eri-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Eri-08-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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
SExtractor catalog cache: saved Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.cat to cache
SExtractor catalog cache: saved Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Creating symlink local_wcs_cache/wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
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_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits exists and is non-empty
wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits exists and is non-empty
wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits exists and is non-empty
wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits (1st reference image)
verification OK: wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Image size: 941.7'x627.6' 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: 03:50:26.444 -26:00:02.47 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_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits (1st new image)
verification OK: wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
Image size: 941.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:50:22.426 -26:00:03.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:50:26.444 -26:00:02.47
Second-epoch image center 03:50:22.426 -26:00:03.39
Angular distance between the image centers 0.0150 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits (2nd new image)
verification OK: wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Image size: 941.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:50:23.053 -26:00:16.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:50:26.444 -26:00:02.47
Second-epoch image center 03:50:23.053 -26:00:16.24
Angular distance between the image centers 0.0133 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 03:50:22.426 -26:00:03.39
Second-epoch second image center 03:50:23.053 -26:00:16.24
Angular distance between the image centers 0.00427 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits &> /tmp/tmp.0nDPahoOFZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits &> /tmp/tmp.tnAlkaRBIL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits &> /tmp/tmp.bUtbYOp7tw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits &> /tmp/tmp.m0URlIpgaC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.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_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits and wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits and wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
Found non-empty wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits and wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
The reference image (wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits) and catalog (wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat) found
'wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat' -> 'wcsmag.cat'
Read 29187 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 48.6796 to 66.9268 deg, Dec -31.3495 to -20.2528 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 48.6796 to 66.9268 deg, Dec -31.3495 to -20.2528 deg
Loaded 6126 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): 4577 out of 4863 total matches.
Matched with Tycho-2 4863 out of 29187 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.636700
a=0.000000 b=1.000000 c=22.636700
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.96
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.96
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29187 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 48.6796 to 66.9268 deg, Dec -31.3495 to -20.2528 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 48.6796 to 66.9268 deg, Dec -31.3495 to -20.2528 deg
Loaded 6126 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): 4577 out of 4863 total matches.
Matched with Tycho-2 4863 out of 29187 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Forced-photometry filter: calibrated wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits -> calib.txt_param_ref_wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits (aperture=4.7)
Read 29963 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 48.6817 to 66.9265 deg, Dec -31.3576 to -20.2725 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 48.6817 to 66.9265 deg, Dec -31.3576 to -20.2725 deg
Loaded 6122 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): 4596 out of 4868 total matches.
Matched with Tycho-2 4868 out of 29963 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
Forced-photometry filter: calibrated wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits -> calib.txt_param_ref_wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 51 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
2.0 pix Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
1.8 pix fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
1.9 pix fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Limiting magnitude estimates:
15.0 mag. Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
15.0 mag. Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
12.7 mag. fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
12.9 mag. fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 12.3 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.0nDPahoOFZ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits' -> 'wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
WCS-calibrated image found: wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
Checking if the catalog wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat corresponding to the image wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat corresponding to the image wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits
WCS catalog name: wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1074, bad_region=0, passed=29176
Got 29176 stars (including 28058 good ones) from the SExtractor catalog wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat
util/solve_plate_with_UCAC5 got 29176 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 29176 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 29176 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 29176 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4896 stars left (next iteration limit 5386)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits N_match=4896 sigma_overall_arcsec=0.283 sigma_q1_arcsec=0.331 sigma_q2_arcsec=0.286 sigma_q3_arcsec=0.259 sigma_q4_arcsec=0.261 n_q1=1300 n_q2=1127 n_q3=1314 n_q4=1155 worst_quadrant_to_overall_ratio=1.169
The image catalog is written to wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits -region wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.tnAlkaRBIL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits' -> 'wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
WCS-calibrated image found: wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
Checking if the catalog wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits
WCS catalog name: wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1000, bad_region=17, passed=29954
Got 29954 stars (including 28881 good ones) from the SExtractor catalog wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat
util/solve_plate_with_UCAC5 got 29954 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 4895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 29954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 29954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 29954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4895 stars left (next iteration limit 5384)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits N_match=4895 sigma_overall_arcsec=0.268 sigma_q1_arcsec=0.305 sigma_q2_arcsec=0.265 sigma_q3_arcsec=0.253 sigma_q4_arcsec=0.246 n_q1=1307 n_q2=1130 n_q3=1306 n_q4=1152 worst_quadrant_to_overall_ratio=1.138
The image catalog is written to wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits -region wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.bUtbYOp7tw (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
WCS_IMAGE_NAME=wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
WCS-calibrated image found: wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
Checking if the catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat corresponding to the image wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat corresponding to the image wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
WCS catalog name: wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=54, bad_region=4, passed=4038
Got 4038 stars (including 3976 good ones) from the SExtractor catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat
util/solve_plate_with_UCAC5 got 4038 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 3822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3815 matched stars entering correct_measured_positions(), 3806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3815 matched stars entering correct_measured_positions(), 4028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 3821 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3814 matched stars entering correct_measured_positions(), 4028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 3814 matched stars entering correct_measured_positions(), 4028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 3814 stars left (next iteration limit 4196)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=3814 robust_rms=4.992 arcsec worst_quadrant_rms=48.438 arcsec
SIP_REFIT: SIP order 3 trial: matched=3814 robust_rms=0.854 arcsec worst_quadrant_rms=0.956 arcsec
SIP_REFIT: SIP order 5 trial: matched=3814 robust_rms=0.747 arcsec worst_quadrant_rms=0.837 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3814 robust_rms_before=1.075 arcsec robust_rms_before_corrected=0.772 arcsec robust_rms_after=0.747 arcsec worst_quadrant_rms_before=0.914 worst_quadrant_rms_after=0.837
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.914 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits N_match=3814 sigma_overall_arcsec=0.709 sigma_q1_arcsec=0.691 sigma_q2_arcsec=0.702 sigma_q3_arcsec=0.852 sigma_q4_arcsec=0.722 n_q1=1803 n_q2=1209 n_q3=372 n_q4=430 worst_quadrant_to_overall_ratio=1.201
The image catalog is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits -region wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.m0URlIpgaC (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
WCS_IMAGE_NAME=wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
WCS-calibrated image found: wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Checking if the catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat corresponding to the image wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat corresponding to the image wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
WCS catalog name: wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=52, bad_region=2, passed=4013
Got 4013 stars (including 3955 good ones) from the SExtractor catalog wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat
util/solve_plate_with_UCAC5 got 4013 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 3802 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3793 matched stars entering correct_measured_positions(), 3781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3793 matched stars entering correct_measured_positions(), 3999 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 3801 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3792 matched stars entering correct_measured_positions(), 4000 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 3792 matched stars entering correct_measured_positions(), 4000 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 3792 stars left (next iteration limit 4172)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=3792 robust_rms=5.043 arcsec worst_quadrant_rms=46.687 arcsec
SIP_REFIT: SIP order 3 trial: matched=3792 robust_rms=0.815 arcsec worst_quadrant_rms=0.968 arcsec
SIP_REFIT: SIP order 5 trial: matched=3792 robust_rms=0.727 arcsec worst_quadrant_rms=0.862 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3792 robust_rms_before=1.047 arcsec robust_rms_before_corrected=0.762 arcsec robust_rms_after=0.727 arcsec worst_quadrant_rms_before=0.920 worst_quadrant_rms_after=0.862
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.920 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits N_match=3792 sigma_overall_arcsec=0.682 sigma_q1_arcsec=0.639 sigma_q2_arcsec=0.685 sigma_q3_arcsec=0.821 sigma_q4_arcsec=0.752 n_q1=1850 n_q2=1267 n_q3=296 n_q4=379 worst_quadrant_to_overall_ratio=1.205
The image catalog is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits -region wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.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_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/wcs_fd_Eri-08-Q1b1x1_2026-09-17_05-59-21_20.00sec_-0.00C_LIGHTs_0101.fits
Saving fully-calibrated image wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.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_2026-09-17_CI_Eri-08-Q1b1x1_060049_TTUQ1b1x1_4189807_4CXG8Xgh/wcs_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102.fits
Preparing the HTML report for the field Eri-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:47:35.24 -23:44:30.9: 13.11 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:41:13.52 -25:30:51.8: 12.32 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:59:39.50 -22:50:49.5: 13.11 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:25.77 -22:08:53.7: 13.52 +/- 0.06 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:01:57.18 -23:18:10.8: 13.06 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:32.48 -22:45:04.2: 13.03 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:21.59 -22:41:38.9: 12.92 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:09:43.78 -22:49:07.9: 12.91 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:37:30.33 -23:20:08.1: 12.87 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:02:27.53 -23:20:43.7: 12.87 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:25.77 -22:08:53.7: 13.55 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:41:13.52 -25:30:51.8: 12.35 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:01:57.18 -23:18:10.8: 13.07 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:59:39.50 -22:50:49.5: 13.03 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:47:35.24 -23:44:30.9: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Forced photometry filter KEPT candidate at 04:00:25.77 -22:08:53.7: ref_mag=13.54 +/- 0.04 new_mean_mag=12.4014 delta=1.13 (need > 0.90)
Forced photometry filter KEPT candidate at 03:41:13.52 -25:30:51.8: ref_mag=12.33 +/- 0.01 new_mean_mag=11.3332 delta=1.00 (need > 0.90)
Forced photometry filter KEPT candidate at 04:01:57.18 -23:18:10.8: ref_mag=13.07 +/- 0.03 new_mean_mag=12.0612 delta=1.01 (need > 0.90)
Forced photometry filter KEPT candidate at 03:59:39.50 -22:50:49.5: ref_mag=13.06 +/- 0.03 new_mean_mag=12.1281 delta=0.93 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:32.48 -22:45:04.2: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter KEPT candidate at 03:47:35.24 -23:44:30.9: ref_mag=13.12 +/- 0.03 new_mean_mag=12.1437 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 04:00:32.48 -22:45:04.2: ref_mag=13.02 +/- 0.02 new_mean_mag=12.0692 delta=0.95 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:21.59 -22:41:38.9: 12.91 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:09:43.78 -22:49:07.9: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 04:00:21.59 -22:41:38.9: ref_mag=12.92 +/- 0.02 new_mean_mag=11.9363 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 04:09:43.78 -22:49:07.9: ref_mag=12.91 +/- 0.02 new_mean_mag=11.8787 delta=1.03 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:37:30.33 -23:20:08.1: 12.77 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter KEPT candidate at 03:37:30.33 -23:20:08.1: ref_mag=12.82 +/- 0.02 new_mean_mag=11.8027 delta=1.01 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:02:27.53 -23:20:43.7: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 04:02:27.53 -23:20:43.7: ref_mag=12.91 +/- 0.02 new_mean_mag=11.9404 delta=0.97 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:47:18.30 -23:43:23.2: 12.86 +/- 0.03 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:47:18.30 -23:43:23.2: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry filter KEPT candidate at 03:47:18.30 -23:43:23.2: ref_mag=12.79 +/- 0.02 new_mean_mag=11.8536 delta=0.94 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:49:43.52 -24:07:24.4: 12.61 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:49:43.52 -24:07:24.4: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Forced photometry filter KEPT candidate at 03:49:43.52 -24:07:24.4: ref_mag=12.60 +/- 0.02 new_mean_mag=11.6434 delta=0.96 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:40:29.21 -25:32:24.0: 12.58 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:38:43.38 -25:16:35.7: 12.56 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:40:29.43 -25:19:47.5: 12.48 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:40:29.21 -25:32:24.0: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Forced photometry filter KEPT candidate at 03:40:29.21 -25:32:24.0: ref_mag=12.61 +/- 0.02 new_mean_mag=11.5784 delta=1.03 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:47:30.86 -23:37:04.0: 12.43 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:38:43.38 -25:16:35.7: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry filter KEPT candidate at 03:38:43.38 -25:16:35.7: ref_mag=12.56 +/- 0.02 new_mean_mag=11.5681 delta=0.99 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:40:29.43 -25:19:47.5: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:29.43 -25:19:47.5: ref_mag=12.49 +/- 0.01 new_mean_mag=11.4789 delta=1.01 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:29.63 -22:59:14.9: 12.38 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:40:41.66 -25:33:30.0: 13.56 +/- 0.06 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:47:30.86 -23:37:04.0: 12.42 +/- 0.02 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:38:20.74 -23:29:32.8: 13.56 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 03:47:30.86 -23:37:04.0: ref_mag=12.42 +/- 0.01 new_mean_mag=11.5052 delta=0.92 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:01:56.06 -23:19:33.3: 13.48 +/- 0.06 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:29.63 -22:59:14.9: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 04:00:29.63 -22:59:14.9: ref_mag=12.38 +/- 0.01 new_mean_mag=11.3828 delta=1.00 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:40:41.66 -25:33:30.0: 13.45 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:38:20.74 -23:29:32.8: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Forced photometry filter KEPT candidate at 03:40:41.66 -25:33:30.0: ref_mag=13.50 +/- 0.04 new_mean_mag=12.3336 delta=1.17 (need > 0.90)
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter KEPT candidate at 03:38:20.74 -23:29:32.8: ref_mag=13.48 +/- 0.04 new_mean_mag=12.3485 delta=1.14 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:01:56.06 -23:19:33.3: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter KEPT candidate at 04:01:56.06 -23:19:33.3: ref_mag=13.48 +/- 0.04 new_mean_mag=12.2558 delta=1.22 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:47:58.22 -23:36:36.0: 13.44 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:47:58.22 -23:36:36.0: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Forced photometry filter KEPT candidate at 03:47:58.22 -23:36:36.0: ref_mag=13.46 +/- 0.04 new_mean_mag=12.2885 delta=1.17 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:40:02.17 -25:33:20.0: 13.39 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:40:02.17 -25:33:20.0: 13.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Forced photometry filter KEPT candidate at 03:40:02.17 -25:33:20.0: ref_mag=13.44 +/- 0.04 new_mean_mag=12.1677 delta=1.27 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:49:49.00 -24:04:00.2: 13.38 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:49:49.00 -24:04:00.2: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 03:49:49.00 -24:04:00.2: ref_mag=13.39 +/- 0.03 new_mean_mag=12.3562 delta=1.04 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:37:44.31 -23:17:58.2: 13.25 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 03:48:28.52 -23:34:51.2: 13.27 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:09:55.61 -22:49:06.2: 13.18 +/- 0.05 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-17_21-08-01_20.00sec_-14.90C_LIGHT_0076.fits at 04:00:44.65 -22:58:13.0: 13.19 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:37:44.31 -23:17:58.2: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter KEPT candidate at 03:37:44.31 -23:17:58.2: ref_mag=13.27 +/- 0.03 new_mean_mag=12.3199 delta=0.95 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 03:48:28.52 -23:34:51.2: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter KEPT candidate at 03:48:28.52 -23:34:51.2: ref_mag=13.27 +/- 0.03 new_mean_mag=12.3258 delta=0.94 (need > 0.90)
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:09:55.61 -22:49:06.2: 13.15 +/- 0.04 detection
Forced photometry on wcs_Eri-08-Q1b1x1_2026-01-20_20-44-31_20.00sec_-15.00C_LIGHT_0083.fits at 04:00:44.65 -22:58:13.0: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry filter KEPT candidate at 04:09:55.61 -22:49:06.2: ref_mag=13.16 +/- 0.03 new_mean_mag=12.0384 delta=1.13 (need > 0.90)
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Forced photometry filter KEPT candidate at 04:00:44.65 -22:58:13.0: ref_mag=13.21 +/- 0.03 new_mean_mag=12.0881 delta=1.13 (need > 0.90)
Adding exclusion_list_local.txt__out04426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13915.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 35s
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: 11s
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Considering the candidate 32507_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32507_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 32514_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32514_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 32515_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32515_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 32520_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32520_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 32523_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32523_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 32524_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32524_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 32530_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32530_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 32531_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32531_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 32532_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32532_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 32538_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32538_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 32540_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32540_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 32542_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32542_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 32552_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32552_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 32553_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32553_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 32565_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32565_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 32567_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32567_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 32570_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32570_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 32579_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32579_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 32590_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32590_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 32592_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32592_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
**** FOUND 03:53:49.70 -24:35:19.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32597_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32597_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 32605_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32605_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 32606_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 32606_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 04426_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 04426_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 13785_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 13785_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 05996_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
The candidate 05996_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102 did not pass the final checks
**** FOUND 03:54:18.04 -22:47:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08602_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 08602_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 06374_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 06374_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 07791_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 07791_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 06104_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 06104_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 05915_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 05915_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 06723_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 06723_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 07311_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 07311_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 07922_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 07922_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 08540_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 08540_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 09791_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 09791_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 13845_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 13845_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 13082_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 13082_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 13241_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 13241_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 08262_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 08262_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 06816_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 06816_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 13915_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 13915_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 07783_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 07783_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 07852_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 07852_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 08277_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 08277_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 13891_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 13891_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 09648_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 09648_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 07208_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 07208_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
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Considering the candidate 08199_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 08199_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06801_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 06801_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06733_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
Preparing report for the candidate 06733_fd_Eri-08-Q1b1x1_2026-09-17_06-00-03_20.00sec_0.00C_LIGHTs_0102
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 48s
Prepared the HTML report for the field Eri-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:00:25.77 -22:08:53.7
04:00:21.59 -22:41:38.9
04:00:32.48 -22:45:04.2
03:59:39.50 -22:50:49.5
04:09:43.78 -22:49:07.9
04:09:55.61 -22:49:06.2
04:00:44.65 -22:58:13.0
04:00:29.63 -22:59:14.9
03:37:44.31 -23:17:58.2
03:37:30.33 -23:20:08.1
03:38:20.74 -23:29:32.8
04:01:57.18 -23:18:10.8
04:01:56.06 -23:19:33.3
04:02:27.53 -23:20:43.7
03:48:28.52 -23:34:51.2
03:47:30.86 -23:37:04.0
03:47:58.22 -23:36:36.0
03:47:18.30 -23:43:23.2
03:47:35.24 -23:44:30.9
03:49:49.00 -24:04:00.2
03:49:43.52 -24:07:24.4
03:38:43.38 -25:16:35.7
03:40:29.43 -25:19:47.5
03:41:13.52 -25:30:51.8
03:40:29.21 -25:32:24.0
03:40:02.17 -25:33:20.0
03:40:41.66 -25:33:30.0
########### Completed Eri-08-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 ####
04:00:25.77 -22:08:53.7
03:41:13.52 -25:30:51.8
03:47:35.24 -23:44:30.9
03:59:39.50 -22:50:49.5
04:01:57.18 -23:18:10.8
04:00:32.48 -22:45:04.2
04:00:21.59 -22:41:38.9
04:09:43.78 -22:49:07.9
03:37:30.33 -23:20:08.1
04:02:27.53 -23:20:43.7
03:47:18.30 -23:43:23.2
03:49:43.52 -24:07:24.4
03:40:29.21 -25:32:24.0
03:38:43.38 -25:16:35.7
03:40:29.43 -25:19:47.5
03:47:30.86 -23:37:04.0
04:00:29.63 -22:59:14.9
03:40:41.66 -25:33:30.0
03:38:20.74 -23:29:32.8
04:01:56.06 -23:19:33.3
03:47:58.22 -23:36:36.0
03:40:02.17 -25:33:20.0
03:49:49.00 -24:04:00.2
03:37:44.31 -23:17:58.2
03:48:28.52 -23:34:51.2
04:00:44.65 -22:58:13.0
04:09:55.61 -22:49:06.2
###################################################################################
04:00:25.77 -22:08:53.7 -- not an asteroid (will add it to exclusion list)
03:41:13.52 -25:30:51.8 -- not an asteroid (will add it to exclusion list)
03:47:35.24 -23:44:30.9 -- not an asteroid (will add it to exclusion list)
03:59:39.50 -22:50:49.5 -- not an asteroid (will add it to exclusion list)
04:01:57.18 -23:18:10.8 -- not an asteroid (will add it to exclusion list)
04:00:32.48 -22:45:04.2 -- not an asteroid (will add it to exclusion list)
04:00:21.59 -22:41:38.9 -- not an asteroid (will add it to exclusion list)
04:09:43.78 -22:49:07.9 -- not an asteroid (will add it to exclusion list)
03:37:30.33 -23:20:08.1 -- not an asteroid (will add it to exclusion list)
04:02:27.53 -23:20:43.7 -- not an asteroid (will add it to exclusion list)
03:47:18.30 -23:43:23.2 -- not an asteroid (will add it to exclusion list)
03:49:43.52 -24:07:24.4 -- not an asteroid (will add it to exclusion list)
03:40:29.21 -25:32:24.0 -- not an asteroid (will add it to exclusion list)
03:38:43.38 -25:16:35.7 -- not an asteroid (will add it to exclusion list)
03:40:29.43 -25:19:47.5 -- not an asteroid (will add it to exclusion list)
03:47:30.86 -23:37:04.0 -- not an asteroid (will add it to exclusion list)
04:00:29.63 -22:59:14.9 -- not an asteroid (will add it to exclusion list)
03:40:41.66 -25:33:30.0 -- not an asteroid (will add it to exclusion list)
03:38:20.74 -23:29:32.8 -- not an asteroid (will add it to exclusion list)
04:01:56.06 -23:19:33.3 -- not an asteroid (will add it to exclusion list)
03:47:58.22 -23:36:36.0 -- not an asteroid (will add it to exclusion list)
03:40:02.17 -25:33:20.0 -- not an asteroid (will add it to exclusion list)
03:49:49.00 -24:04:00.2 -- not an asteroid (will add it to exclusion list)
03:37:44.31 -23:17:58.2 -- not an asteroid (will add it to exclusion list)
03:48:28.52 -23:34:51.2 -- not an asteroid (will add it to exclusion list)
04:00:44.65 -22:58:13.0 -- not an asteroid (will add it to exclusion list)
04:09:55.61 -22:49:06.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:37:30.33 -23:20:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:44.31 -23:17:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:20.74 -23:29:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:43.38 -25:16:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:02.17 -25:33:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:29.21 -25:32:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:29.43 -25:19:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:41.66 -25:33:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:13.52 -25:30:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:18.30 -23:43:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:30.86 -23:37:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:35.24 -23:44:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:58.22 -23:36:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:28.52 -23:34:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:43.52 -24:07:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:49.00 -24:04:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:59:39.50 -22:50:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:21.59 -22:41:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:25.77 -22:08:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:29.63 -22:59:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:32.48 -22:45:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:44.65 -22:58:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:56.06 -23:19:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:57.18 -23:18:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:27.53 -23:20:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:09:43.78 -22:49:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:09:55.61 -22:49:06.2 -- 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)
03:37:30.33 -23:20:08.1 -- not a known variable star
03:37:44.31 -23:17:58.2 -- not a known variable star
03:38:20.74 -23:29:32.8 -- not a known variable star
03:38:43.38 -25:16:35.7 -- not a known variable star
03:40:02.17 -25:33:20.0 -- not a known variable star
03:40:29.21 -25:32:24.0 -- not a known variable star
03:40:29.43 -25:19:47.5 -- not a known variable star
03:40:41.66 -25:33:30.0 -- not a known variable star
03:41:13.52 -25:30:51.8 -- not a known variable star
03:47:18.30 -23:43:23.2 -- not a known variable star
03:47:30.86 -23:37:04.0 -- not a known variable star
03:47:35.24 -23:44:30.9 -- not a known variable star
03:47:58.22 -23:36:36.0 -- a known variable star
03:48:28.52 -23:34:51.2 -- not a known variable star
03:49:43.52 -24:07:24.4 -- not a known variable star
03:49:49.00 -24:04:00.2 -- not a known variable star
03:59:39.50 -22:50:49.5 -- not a known variable star
04:00:21.59 -22:41:38.9 -- not a known variable star
04:00:25.77 -22:08:53.7 -- not a known variable star
04:00:29.63 -22:59:14.9 -- not a known variable star
04:00:32.48 -22:45:04.2 -- not a known variable star
04:00:44.65 -22:58:13.0 -- not a known variable star
04:01:56.06 -23:19:33.3 -- not a known variable star
04:01:57.18 -23:18:10.8 -- not a known variable star
04:02:27.53 -23:20:43.7 -- a known variable star
04:09:43.78 -22:49:07.9 -- not a known variable star
04:09:55.61 -22:49:06.2 -- not a known variable star
Found 25 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
27 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 ####
03:37:30.33 -23:20:08.1
03:37:44.31 -23:17:58.2
03:38:20.74 -23:29:32.8
03:38:43.38 -25:16:35.7
03:40:02.17 -25:33:20.0
03:40:29.21 -25:32:24.0
03:40:29.43 -25:19:47.5
03:40:41.66 -25:33:30.0
03:41:13.52 -25:30:51.8
03:47:18.30 -23:43:23.2
03:47:30.86 -23:37:04.0
03:47:35.24 -23:44:30.9
03:47:58.22 -23:36:36.0
03:48:28.52 -23:34:51.2
03:49:43.52 -24:07:24.4
03:49:49.00 -24:04:00.2
03:59:39.50 -22:50:49.5
04:00:21.59 -22:41:38.9
04:00:25.77 -22:08:53.7
04:00:29.63 -22:59:14.9
04:00:32.48 -22:45:04.2
04:00:44.65 -22:58:13.0
04:01:56.06 -23:19:33.3
04:01:57.18 -23:18:10.8
04:02:27.53 -23:20:43.7
04:09:43.78 -22:49:07.9
04:09:55.61 -22:49:06.2
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461300.95800641 -observatory V36
12:39:07.95 -04:16:27.9 Mercury (-0.4mag)
13:58:19.95 -17:58:20.5 Venus (-4.8mag)
07:40:56.27 +22:12:44.8 Mars (1.2mag)
09:17:12.80 +16:22:29.0 Jupiter (-1.8mag)
00:49:12.51 +02:21:06.7 Saturn (0.4mag)
04:13:37.76 +21:01:51.5 Uranus (5.7mag)
00:12:45.28 -00:09:52.3 Neptune (7.7mag)
20:24:58.00 -23:41:36.9 Pluto (14.5mag)
16:24:17.04 -26:57:12.1 Moon (-10.0mag)
-rw-r--r-- 1 apache apache 363 Sep 17 06:01 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461300.95800641:
09:17:19.54 +16:21:55.4 Io (6.0mag)
09:17:17.10 +16:22:08.3 Europa (6.2mag)
09:16:59.87 +16:23:37.2 Ganymede (5.6mag)
09:17:28.97 +16:21:07.1 Callisto (6.8mag)
09:15:24.50 +16:42:43.6 Himalia (15.7mag)
09:17:16.91 +16:22:09.6 Thebe (16.5mag)
09:14:52.73 +16:36:53.3 Elara (17.7mag)
09:20:48.76 +15:47:25.4 Pasiphae (17.9mag)
09:17:33.46 +16:43:04.9 Carme (18.9mag)
00:49:23.58 +02:20:39.9 Titan (8.3mag)
00:49:13.19 +02:20:46.1 Rhea (9.6mag)
00:48:58.54 +02:22:06.6 Iapetus (11.0mag)
00:48:58.84 +02:21:21.0 Hyperion (14.3mag)
00:47:49.28 +02:09:59.2 Phoebe (16.3mag)
-rw-r--r-- 1 apache apache 568 Sep 17 06:02 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461300.95800641:
23:29:38.21 +10:55:43.6 JWST
17:02:10.47 +41:14:10.1 Chandra
13:18:00.53 -62:23:23.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 17 06:01 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461300.95800641 -observatory V36
03:45:16.06 +19:44:56.2 17.3mag P/1996 R2 (Lagerkvist)
18:07:25.42 -34:00:56.7 14.5mag P/2010 H2 (Vales)
07:26:44.87 -70:53:11.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:32.79 +33:58:14.6 17.7mag C/2017 K2 (PANSTARRS)
05:02:39.08 +46:47:37.6 16.2mag P/2021 N1 (ZTF)
22:05:43.15 +27:21:44.9 17.5mag C/2022 E2 (ATLAS)
07:17:26.73 +25:47:43.8 16.9mag C/2022 N2 (PANSTARRS)
10:58:47.95 +26:53:11.0 17.1mag C/2022 QE78 (ATLAS)
09:55:00.08 +05:10:32.2 18.0mag C/2022 R6 (PANSTARRS)
15:27:36.76 -16:32:11.9 15.0mag C/2023 R1 (PANSTARRS)
08:46:48.29 +33:34:04.7 15.9mag C/2024 E1 (Wierzchos)
15:08:15.64 +15:12:48.7 18.0mag C/2024 G6 (ATLAS)
18:28:30.39 +42:43:29.2 13.7mag C/2024 J3 (ATLAS)
20:13:05.45 +48:36:55.6 17.4mag C/2024 R4 (PANSTARRS)
05:40:25.59 -13:11:09.6 15.0mag C/2024 T5 (ATLAS)
07:14:27.93 +16:27:28.6 17.8mag C/2025 J1 (Borisov)
11:34:41.85 +17:57:43.5 16.6mag C/2025 V2 (Rankin)
13:28:17.69 -00:42:55.1 16.7mag C/2025 Y1 (ATLAS)
17:11:26.33 +72:10:10.7 15.9mag C/2026 A2 (Bok)
02:59:28.33 +45:41:02.0 17.5mag C/2026 B2 (Sun-Gao)
12:22:46.95 +12:06:55.1 17.6mag A/2026 E1
22:34:37.50 -35:08:23.5 13.6mag 10P/Tempel
01:35:17.84 +38:46:39.1 17.5mag 11P/Tempel-Swift-LINEAR
11:55:01.39 -06:14:45.2 16.3mag 29P/Schwassmann-Wachmann
12:29:01.70 -08:16:21.7 17.8mag 63P/Wild
06:58:15.47 +18:24:31.8 17.1mag 78P/Gehrels
03:16:07.42 +15:01:40.7 17.3mag 88P/Howell
06:12:47.33 +32:25:39.1 17.3mag 112P/Urata-Niijima
08:01:07.63 +22:01:23.4 17.8mag 114P/Wiseman-Skiff
10:50:20.00 +18:40:11.6 14.8mag 123P/West-Hartley
13:09:22.66 -24:48:13.2 17.5mag 124P/Mrkos
06:29:07.50 +20:17:40.0 15.8mag 128P/Shoemaker-Holt
01:37:51.24 -15:28:42.6 14.5mag 161P/Hartley-IRAS
09:32:34.75 +08:38:50.9 12.5mag 169P/NEAT
03:30:56.87 +07:30:53.9 14.6mag 220P/McNaught
05:14:26.45 +39:19:49.4 15.3mag 260P/McNaught
08:58:22.79 +34:32:17.7 17.3mag 295P/LINEAR
15:32:15.78 -01:22:43.5 17.9mag 391P/Kowalski
09:36:24.56 +16:20:10.7 17.8mag 450P/LONEOS
-rw-r--r-- 1 apache apache 1.9K Sep 17 06:01 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:21:12.24 +57:37:51.30 SN 2026aafh 2026-09-14.11 15.02
23:36:00.27 -19:28:18.00 SN 2026aaks 2026-09-14.44 16.89
16:35:24.86 -05:32:38.20 SN2026aasi 2026-09-12.99 16.58
16:46:08.71 +37:25:21.80 SN2026aafk 2026-09-13.25 17.4
23:48:37.86 +50:25:24.60 SN2026aafs 2026-09-13.47 17
21:20:27.02 +02:10:42.50 SN2026aagh -------
08:02:26.85 -24:37:44.10 ASASSN-26fe 2026-09-13.34 13.67
02:29:34.91 +23:06:56.30 SN2026aars 2026-09-12.27 16.93
02:47:25.52 -32:58:34.50 SN 2026znh 2026-09-9.92 16.26
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc 2026-09-8.79 12.14
03:52:53.26 -14:19:28.70 SN 2026zfw 2026-09-8 17.78
01:53:26.46 +10:07:25.10 SN2026aacj 2026-09-7.17 16.27
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.59 +34:24:35.70 SN2026aaiv 2026-09-7.22 13.48
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa 2026-08-31.18 14.63
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.79 -22:25:29.10 V8055 2026-08-30 10.76
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
-rw-r--r-- 1 apache apache 190K Sep 17 06:01 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
23:02:59.000 +04:07:07.54 AT 2026zte 2026-08-06.81 22.32
01:13:09.050 +05:20:55.79 AT 2026ztd 2026-08-14.81 22.13
02:07:04.940 +06:29:48.96 AT 2026ztc 2026-08-09.87 22.6
00:13:27.510 -00:06:02.69 AT 2026ztb 2026-08-11.76 22.12
23:15:50.170 -00:21:47.12 AT 2026zta 2026-08-18.74 22.24
02:46:12.842 +06:11:52.33 AT 2026zsz 2026-08-23.78 19.3
22:38:13.667 +15:06:36.55 AT 2026zsy 2026-08-19.88 18.99
16:29:10.420 +50:17:23.09 SN 2026zsx 2026-08-23.92 18.643
00:30:37.105 +16:40:45.90 AT 2026zsw 2026-08-22.04 19.582
00:15:59.164 +45:15:18.02 AT 2026zsv 2026-08-15.37 21.2462
18:01:12.850 +23:06:59.14 AT 2026zsu 2026-08-12.17 20.552
16:34:01.788 +10:33:21.97 AT 2026zst 2026-08-05.18 20.8897
07:35:51.970 +14:30:02.34 AT 2026zss 2026-08-23.51 19.3532
12:34:19.746 +36:30:42.03 AT 2026zsr 2026-08-18.15 16.215
13:54:24.090 +08:32:46.11 AT 2026zsq 2026-08-17.15 19.6164
14:02:03.482 +00:12:24.13 AT 2026zsp 2026-08-18.15 20.1377
14:26:57.209 +16:14:29.77 AT 2026zso 2026-08-18.15 19.8733
15:19:36.047 +10:32:58.31 AT 2026zsn 2026-08-24.15 19.7907
14:53:08.508 -01:21:20.01 AT 2026zsm 2026-08-06.17 20.2832
23:26:24.962 -03:37:54.53 AT 2026zsl 2026-08-22.08 20.35
-rw-r--r-- 1 apache apache 89K Sep 17 06:01 tns_transients_list.txt
