This analysis is done by the script util/transients/transient_factory_test31.sh /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI
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:
2025 12 27.1066 2461036.6066 11.35 03:57:29.29 -06:40:06.4
196.80705 -41.39854 galactic Eri Second-epoch detections are separated by 2.8" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3244886519850034816 | 03:57:29.83 -06:40:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.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 2025 12 27.1066* 03 57 29.29 -06 40 06.4 11.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3244886519850034816,2461036.6066,11.35,0.05,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
Gaia DR3 3244886519850034816 20251227.1066 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:29.29 -06:40:06.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 38 32.66 +01 14 24.2 12.4 U Tau 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461036.6066,12.37,0.05,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
VARIABLE_NAME 20251227.1066 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:32.66 +01:14:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 04 23.05 +02 57 45.0 12.3 U Cet 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,12.29,0.05,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
target 20251227.1066 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:04:23.05 +02:57:45.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 02 58 58.01 +00 17 23.1 12.7 U Cet 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,12.68,0.05,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 20251227.1066 12.68CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:58.01 +00:17:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 51 16.73 -04 20 31.9 13.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,13.06,0.05,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 20251227.1066 13.06CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:16.73 -04:20:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 02 56 33.77 +02 06 56.7 13.1 U Cet 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.1066 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:33.77 +02:06:56.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 56 39.02 +03 01 57.5 13.4 U Tau 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,13.41,0.05,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 20251227.1066 13.41CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:39.02 +03:01:57.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 44 20.67 +00 17 15.1 13.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461036.6066,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20251227.1066 13.42CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:20.67 -00:17:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 10 06.26 +00 11 25.9 13.5 U Cet 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,13.48,0.05,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 20251227.1066 13.48CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:10:06.26 -00:11:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 00 38.10 -01 34 44.8 14.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.1066 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:38.10 -01:34:44.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 55 54.40 -06 26 09.5 14.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.1066 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:54.40 -06:26:09.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 21 01.05 +02 27 22.9 14.3 U Cet 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.1066 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:01.05 +02:27:22.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 02 03.36 -01 16 12.7 14.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.1066 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:02:03.36 -01:16:12.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 12 54.96 +01 55 06.5 14.2 U Cet 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.1066 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:12:54.96 +01:55:06.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 02 57 05.75 +00 35 01.5 14.3 U Cet 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,14.35,0.05,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 20251227.1066 14.35CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:05.75 -00:35:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 02 57 42.08 +00 46 52.4 14.5 U Cet 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.1066 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:42.08 -00:46:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 03 21.80 -01 19 26.7 14.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,14.49,0.05,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
target 20251227.1066 14.49CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:21.80 -01:19:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
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 2025 12 27.1066* 03 08 05.27 +00 27 00.6 14.5 U Cet 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.6066,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.1066 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:05.27 +00:27:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20_00sec_-15_00C_LIGHT_0179_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v2.gif
Processing complete!
Total number of candidates identified: 18
Processing log:
Images processed 4
Images used for photometry 4
Ref. image: 2461028.71645017 19.12.2025 05:11:31.295 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits
First image: 2461028.71645017 19.12.2025 05:11:31.295 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits
Last image: 2461036.60679870 27.12.2025 02:33:37.408 /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
Estimated ref. image limiting mag.: -10.63
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: 1
User-specified moving object: none
Computation time: 34 seconds
Number of parallel threads: 12
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6527
Objects passed selection criteria: 6522
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 6237.25
Average stars matched: 6136.5 (98.3847 %)
Memory usage VmPeak: 91436 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Thu Dec 25 11:45:33 -00 2025
VaST build number 1.0rc88-81-g00db519e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2025-12-25)
GNU bash, version 5.3.3(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Dec 27 04:32:23 -00 2025
Host name: tau
############################################################
Images processed 4
Images used for photometry 4
Ref. image: 2461028.71645017 19.12.2025 05:11:31.295 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits
First image: 2461028.71645017 19.12.2025 05:11:31.295 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits
Last image: 2461036.60679870 27.12.2025 02:33:37.408 /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 74
Estimated ref. image limiting mag.: -7.99
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: 1
User-specified moving object: none
Computation time: 67 seconds
Number of parallel threads: 12
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 2.1 # or , in mag.arcsec-2
ANALYSIS_THRESH 2.1 # or , in mag.arcsec-2
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 34360
Objects passed selection criteria: 34276
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 33092.8
Average stars matched: 32204.8 (97.3166 %)
Memory usage VmPeak: 114780 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Thu Dec 25 11:45:33 -00 2025
VaST build number 1.0rc88-81-g00db519e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2025-12-25)
GNU bash, version 5.3.3(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Dec 27 04:35:57 -00 2025
Host name: tau
############################################################
Filtering log:
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst
CAMERA_SETTINGS= TTUQ1b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR= /var/www/nmw_calibration/TTUQ1b1x1/darks
EXCLUSION_LIST= ../exclusion_list_TTUQ1.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE= /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
FRAME_EDGE_OFFSET_PIX= 50
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS= 12
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= no
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 1
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
Reference image directory is set to /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved
VIZIER_SITE=vizier.cds.unistra.fr
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
Fields in the data directory:
Eri-01-Q1b1x1
#######################################
########### Starting Eri-01-Q1b1x1 ###########
Processing Eri-01-Q1b1x1
server tau has sufficient free disk space available: 574930 MB at /mnt/usb2/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 574930 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits
REFERENCE_EPOCH__SECOND_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png' -> 'transient_report/Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits_preview.png'
Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
renamed 'Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png' -> 'transient_report/Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits_preview.png'
Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
Read-check the input FITS images... read-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 776.1724
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 532.4187
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1557.0976
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 614.3105
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1555.4465
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 613.2289
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.00612
INFO: SECOND_EPOCH__SD_ratio= 0.002
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR=/var/www/nmw_calibration/TTUQ1b1x1/darks FLAT_FIELD_FILE=/var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -15.0 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2025-12-26T20:33:02.9995032' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2025-12-27T02:33:02.9995032' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61036.1062847106 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2025-12-27T02:33:12.9026766' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61036.1063993289 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -15.0 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 51.4278441297695 / [deg] RA of telescope" status=0
Record 32: "DEC = -1.99972295954415 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 49.8788888888889 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 148.756666666667 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.30678553342699 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'West' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Eri-01' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '03 25 43' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '-02 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/d_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits :)
Spent 0.462547 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2025-12-22.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/d_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -14.9 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2025-12-26T20:33:37.4088886' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2025-12-27T02:33:37.4088886' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61036.1066829627 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2025-12-27T02:33:47.3120312' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61036.1067975927 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -14.9 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 51.4278441476255 / [deg] RA of telescope" status=0
Record 32: "DEC = -1.99972294539334 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 49.94 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 148.955833333333 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.30561632652262 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'West' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Eri-01' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '03 25 43' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '-02 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/d_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits :)
Spent 0.418811 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2025-12-22.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/d_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
Dark frame used to calibrate the second-epoch images:
Flat field used to calibrate the second-epoch images:
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
Previews of the CALIBRATED second-epoch images:
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 1 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.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: 2461036.60640045
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits exists and is non-empty
Saving wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits to local_wcs_cache/
'wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits' -> 'local_wcs_cache/wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits'
wcs_Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits exists and is non-empty
Saving wcs_Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits to local_wcs_cache/
'wcs_Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits' -> 'local_wcs_cache/wcs_Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits'
wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits exists and is non-empty
Saving wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits to local_wcs_cache/
'wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits' -> 'local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits'
wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits exists and is non-empty
Saving wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits to local_wcs_cache/
'wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits' -> 'local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:25:43.335 -02:00:10.92
Second-epoch image center 03:26:06.918 -02:00:26.91
Angular distance between the image centers 0.10 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:25:43.335 -02:00:10.92
Second-epoch image center 03:26:06.423 -02:00:28.11
Angular distance between the image centers 0.10 deg.
###################################
Running solve_plate_with_UCAC5
Calibrating the magnitude scale
Found non-empty wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.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-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat
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-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat
Found non-empty wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat
The reference image (wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits) and catalog (wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat) found
'wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3880 out of 6595 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.806009
a=0.000000 b=1.000000 c=22.806009
From vast_summary.log: estimated ref. image limiting mag.: -10.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.18
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.18
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits
2.1 pix Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits
2.5 pix fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
2.5 pix fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
All-image limiting magnitude estimate: 11.9 with default.sex.telephoto_lens_onlybrightstars_v1
(80th percentile of magnitude distribution of stars detected on all four images)
Waiting for UCAC5 plate solver
wait
Copying WCS-calibrated images back to input directory
'wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits'
'wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits'
Preparing the HTML report for the field Eri-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20228.dat to exclusion_list_local.txt
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20202_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 20202_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20228_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 20228_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/20228_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/20228_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/20228_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20238_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 20238_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
**** FOUND 03:34:43.59 -02:16:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20239_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 20239_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
**** FOUND 03:48:42.99 -02:58:47.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20243_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 20243_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
**** FOUND 03:33:26.05 -01:29:30.8 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.14 -c=03:33:26.05 -01:29:30.8 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 1.594 3262984172004414336 053.35895426103 -01.49172805539 11.9845 11.5160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
Prepared the HTML report for the field Eri-01-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 ####
03:57:29.29 -06:40:06.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 1 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits
Creating symlink local_wcs_cache/wcs_Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Creating symlink local_wcs_cache/exclusion_list_bsc.txt
Creating symlink local_wcs_cache/exclusion_list_tycho2.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits exists and is non-empty
wcs_Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:25:43.335 -02:00:10.92
Second-epoch image center 03:26:06.918 -02:00:26.91
Angular distance between the image centers 0.10 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:25:43.335 -02:00:10.92
Second-epoch image center 03:26:06.423 -02:00:28.11
Angular distance between the image centers 0.10 deg.
###################################
Running solve_plate_with_UCAC5
Calibrating the magnitude scale
Found non-empty wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.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-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat
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-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat
Found non-empty wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat
The reference image (wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits) and catalog (wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat) found
'wcs_Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 4010 out of 34918 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.683310
a=0.000000 b=1.000000 c=22.683310
From vast_summary.log: estimated ref. image limiting mag.: -7.99
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.69
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.69
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits
2.0 pix Eri-01-Q1b1x1_2025-12-18_23-12-10_20.00sec_-15.00C_LIGHT_0180.fits
2.3 pix fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits
2.3 pix fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits
All-image limiting magnitude estimate: 14.4 with default.sex.telephoto_lens_vSTL
(80th percentile of magnitude distribution of stars detected on all four images)
Waiting for UCAC5 plate solver
wait
Copying WCS-calibrated images back to input directory
'wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.fits'
'wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_Eri-01-Q1b1x1_222822_TTUQ1b1x1_5821_eylTLMkI/wcs_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.fits'
Preparing the HTML report for the field Eri-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52621.dat to exclusion_list_local.txt
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Considering the candidate 52381_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52381_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
**** FOUND 03:48:48.54 -02:35:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52384_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52384_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 52387_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52387_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (30.8") between the two second-epoch detections
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Considering the candidate 52389_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52389_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
**** FOUND 03:40:30.43 +00:05:01.8 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.00, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..11.98 -c=03:40:30.43 +00:05:01.8 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
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Considering the candidate 52417_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52417_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
**** FOUND 03:57:29.44 -06:40:07.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52434_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52434_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52434_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52434_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52434_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52436_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52436_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
**** FOUND 03:50:16.90 -01:32:59.3 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.42 -c=03:50:16.90 -01:32:59.3 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 2.987 3250457676549740288 057.57124640089 -01.54978703839 12.1677 11.4353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52438_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52438_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52438_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52438_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52438_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52450_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52450_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
**** FOUND 03:57:23.67 -04:47:56.5 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.66 -c=03:57:23.67 -04:47:56.5 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 3.870 3245778734879729408 059.34969911888 -04.79912835569 12.5563 12.0963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52457_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52457_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52457_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52457_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52457_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52461_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52461_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52461_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52461_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52461_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52473_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52473_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52473_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52473_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52473_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52475_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52475_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52475_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52475_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52475_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52485_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52485_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52485_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52485_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52485_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52488_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52488_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52499_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52499_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52499_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52499_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52499_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52503_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52503_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 52507_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52507_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (36.8") between the two second-epoch detections
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Considering the candidate 52513_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52513_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (34.8") between the two second-epoch detections
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Considering the candidate 52514_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52514_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
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Considering the candidate 52522_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52522_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52522_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52522_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52522_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52533_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52533_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52533_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52533_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52533_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52536_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52536_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 52552_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52552_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 52553_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52553_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52553_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52553_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52553_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52558_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52558_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52558_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52558_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52558_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52566_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52566_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52566_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52566_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52566_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52568_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52568_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (34.9") between the two second-epoch detections
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Considering the candidate 52586_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52586_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52586_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52586_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52586_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52595_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52595_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 52603_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52603_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52603_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52603_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52603_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52610_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 52610_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks
Rejecting candidate due to large distance (34.3") between the two second-epoch detections
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Considering the candidate 52616_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52616_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52616_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52616_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52616_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 52621_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Preparing report for the candidate 52621_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
Successfully moved Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.png to transient_report/52621_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_reference.png
The output file transient_report/Eri-01-Q1b1x1_2025-12-18_23-11-31_20.00sec_-15.00C_LIGHT_0179.fits_preview.png already exist
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-02_20.00sec_-15.00C_LIGHT_0087.png to transient_report/52621_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery1.png
Successfully moved fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088.png to transient_report/52621_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088_discovery2.png
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Considering the candidate 33819_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088
The candidate 33819_fd_Eri-01-Q1b1x1_2025-12-26_20-33-37_20.00sec_-14.90C_LIGHT_0088 did not pass the final checks