This analysis is done by the script util/transients/transient_factory_test31.sh /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut
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 23.2631 2461032.7631 11.24 05:03:58.50 -03:30:13.1
203.28903 -25.42321 galactic Ori Second-epoch detections are separated by 1.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3213178391212584960 | 05:03:59.41 -03:29:51.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.771+/-0.033 (K)
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 23.2631* 05 03 58.50 -03 30 13.1 11.2 U Ori 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 3213178391212584960,2461032.7631,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3213178391212584960 20251223.2631 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:58.50 -03:30:13.1 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.88 05:01:21.54 -00:43:16.5
200.25500 -24.64091 galactic Ori Second-epoch detections are separated by 0.2" and 8.4 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 3227246535112872192 | 05:01:21.43 -00:43:16.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.033 (G)
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 23.2631* 05 01 21.54 +00 43 16.5 11.9 U Ori 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 3227246535112872192,2461032.7631,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3227246535112872192 20251223.2631 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:21.54 -00:43:16.5 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 26 08.97 +00 49 41.7 11.9 U Ori 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 3221876073646004864,2461032.7631,11.94,0.05,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 3221876073646004864 20251223.2631 11.94CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:08.97 +00:49:41.7 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.93 05:18:18.85 +02:23:51.5
199.61153 -19.41299 galactic Ori Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3234486990980293504 | 05:18:18.28 +02:23:15.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.036 (G)
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 23.2631* 05 18 18.85 +02 23 51.5 11.9 U Ori 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 3234486990980293504,2461032.7631,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3234486990980293504 20251223.2631 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:18.85 +02:23:51.5 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.91 05:11:57.50 -01:32:24.6
202.45103 -22.73151 galactic Ori Second-epoch detections are separated by 1.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3215308587614324096 | 05:11:57.36 -01:32:24.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.231+/-0.031 (F)
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 23.2631* 05 11 57.50 -01 32 24.6 11.9 U Ori 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 3215308587614324096,2461032.7631,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3215308587614324096 20251223.2631 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:57.50 -01:32:24.6 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.94 05:17:15.56 -01:58:34.8
203.55193 -21.77926 galactic Ori Second-epoch detections are separated by 0.6" and 8.4 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 3214294322498070528 | 05:17:15.46 -01:58:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.537+/-0.029 (K)
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 23.2631* 05 17 15.56 -01 58 34.8 11.9 U Ori 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 3214294322498070528,2461032.7631,11.94,0.05,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 3214294322498070528 20251223.2631 11.94CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:15.56 -01:58:34.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 35 31.99 -05 09 28.0 12.0 U Ori 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
V0360 Ori,2461032.7631,11.98,0.05,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
V0360 Ori 20251223.2631 11.98CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:31.99 -05:09:28.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.95 05:08:10.90 -02:40:18.8
203.03724 -24.10324 galactic Ori Second-epoch detections are separated by 0.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.0403-02.6731 | 05:08:10.75 -02:40:18.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 23.2631* 05 08 10.90 -02 40 18.8 11.9 U Ori 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
ATO J077.0403-02.6731,2461032.7631,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.0403-02.6731 20251223.2631 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:08:10.90 -02:40:18.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.94 05:13:09.44 -02:03:25.9
203.09871 -22.71784 galactic Ori Second-epoch detections are separated by 0.5" and 8.3 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 | Large-amplitude variable Gaia DR2 3214703448196923392 | 05:13:09.40 -02:03:26.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.631+/-0.033 (K)
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 23.2631* 05 13 09.44 -02 03 25.9 11.9 U Ori 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
Large-amplitude variable Gaia DR2 3214703448196923392,2461032.7631,11.94,0.05,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
Large-amplitude variable Gaia DR2 3214703448196923392 20251223.2631 11.94CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:09.44 -02:03:25.9 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.99 05:34:42.04 -03:41:56.8
207.35024 -18.73954 galactic Ori Second-epoch detections are separated by 0.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J083.6748-03.6991 | 05:34:41.96 -03:41:56.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.034 (G)
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 23.2631* 05 34 42.04 -03 41 56.8 12.0 U Ori 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
ATO J083.6748-03.6991,2461032.7631,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.6748-03.6991 20251223.2631 11.99CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:42.04 -03:41:56.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 12.04 05:25:53.15 -00:11:55.4
202.99049 -19.03480 galactic Ori Second-epoch detections are separated by 1.0" and 8.4 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 3220632388556032000 | 05:25:52.38 -00:11:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
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 23.2631* 05 25 53.15 +00 11 55.4 12.0 U Ori 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 3220632388556032000,2461032.7631,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3220632388556032000 20251223.2631 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:53.15 -00:11:55.4 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.96 05:12:36.45 -03:15:06.5
204.16922 -23.40765 galactic Ori Second-epoch detections are separated by 0.5" and 8.4 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 3213720347364240384 | 05:12:36.33 -03:15:06.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.595+/-0.035 (K)
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 23.2631* 05 12 36.45 -03 15 06.5 12.0 U Ori 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 3213720347364240384,2461032.7631,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3213720347364240384 20251223.2631 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:36.45 -03:15:06.5 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.96 05:27:31.65 -05:05:21.0
207.79226 -20.96582 galactic Ori Second-epoch detections are separated by 0.1" and 8.4 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 3209354182393987456 | 05:27:31.55 -05:05:20.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.677+/-0.035 (K)
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 23.2631* 05 27 31.65 -05 05 21.0 12.0 U Ori 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 3209354182393987456,2461032.7631,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3209354182393987456 20251223.2631 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:31.65 -05:05:21.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.98 05:16:19.35 -01:52:14.0
203.33125 -21.93428 galactic Ori Second-epoch detections are separated by 0.9" and 8.3 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 3215050206677141888 | 05:16:19.18 -01:52:14.0 (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 23.2631* 05 16 19.35 -01 52 14.0 12.0 U Ori 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 3215050206677141888,2461032.7631,11.98,0.05,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 3215050206677141888 20251223.2631 11.98CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:19.35 -01:52:14.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.96 05:06:26.77 -05:54:18.4
205.96426 -26.00353 galactic Eri Second-epoch detections are separated by 0.4" and 8.4 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 3211314134886300160 | 05:06:26.66 -05:54:18.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.968+/-0.035 (M)
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 23.2631* 05 06 26.77 -05 54 18.4 12.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3211314134886300160,2461032.7631,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3211314134886300160 20251223.2631 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:26.77 -05:54:18.4 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 35 46.71 -05 17 57.2 12.0 U Ori 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,2461032.7631,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20251223.2631 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:46.71 -05:17:57.2 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.97 05:13:25.03 +02:38:35.3
198.73366 -20.34822 galactic Ori Second-epoch detections are separated by 0.4" and 8.4 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 | ATO J078.3599+02.6438 | 05:13:24.82 +02:38:07.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1949AnHar.112....1C HD 287614 J-Ks=0.393+/-0.030 (G)
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 23.2631* 05 13 25.03 +02 38 35.3 12.0 U Ori 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
ATO J078.3599+02.6438,2461032.7631,11.97,0.05,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
ATO J078.3599+02.6438 20251223.2631 11.97CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:25.03 +02:38:35.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 12.03 05:12:13.59 -01:50:31.3
202.77287 -22.81841 galactic Ori Second-epoch detections are separated by 1.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3214725197912733056 | 05:12:13.53 -01:50:31.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949AnHar.112....1C HD 290106 J-Ks=0.207+/-0.031 (F)
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 23.2631* 05 12 13.59 -01 50 31.3 12.0 U Ori 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 3214725197912733056,2461032.7631,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3214725197912733056 20251223.2631 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:13.59 -01:50:31.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 54 00.85 -01 31 14.6 14.4 U Ori 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,2461032.7631,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251223.2631 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:00.85 -01:31:14.6 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 11 13.84 -02 54 33.6 14.5 U Ori 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,2461032.7631,14.49,0.05,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 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:13.84 -02:54:33.6 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 53 10.49 -05 42 38.0 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,2461032.7631,14.46,0.05,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 20251223.2631 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:53:10.49 -05:42:38.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 07 55.91 +01 40 37.1 14.4 U Ori 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 3234787711707855104,2461032.7631,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3234787711707855104 20251223.2631 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:55.91 +01:40:37.1 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.43 05:31:11.63 -02:35:06.7
205.87825 -18.99834 galactic Ori Second-epoch detections are separated by 0.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J082.7967-02.5942 | 05:31:11.63 -02:35:06.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
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 23.2631* 05 31 11.63 -02 35 06.7 14.4 U Ori 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
ATO J082.7967-02.5942,2461032.7631,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.7967-02.5942 20251223.2631 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:11.63 -02:35:06.7 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 17 59.30 +02 23 20.0 14.2 U Ori 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,2461032.7631,14.18,0.05,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 20251223.2631 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:59.30 +02:23:20.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 46 03.76 -02 26 04.3 13.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3226030616988263680,2461032.7631,13.79,0.05,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 3226030616988263680 20251223.2631 13.79CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:03.76 -02:26:04.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 34 51.16 +01 53 18.7 13.8 U Ori 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
CSS_J053450.5+015335,2461032.7631,13.76,0.05,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
CSS_J053450.5+015335 20251223.2631 13.76CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:51.16 +01:53:18.7 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 13.12 05:18:58.95 +01:42:48.4
200.32950 -19.60798 galactic Ori Second-epoch detections are separated by 0.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.7451+01.7135 | 05:18:59.82 +01:42:40.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.533+/-0.030 (K)
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 23.2631* 05 18 58.95 +01 42 48.4 13.1 U Ori 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
ATO J079.7451+01.7135,2461032.7631,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.7451+01.7135 20251223.2631 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:58.95 +01:42:48.4 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 12.85 05:26:37.89 -02:54:15.3
205.61235 -20.15462 galactic Ori Second-epoch detections are separated by 0.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:26:37.89 -02:54:15.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.279+/-0.037 (F)
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 23.2631* 05 26 37.89 -02 54 15.3 12.8 U Ori 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,2461032.7631,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251223.2631 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:37.89 -02:54:15.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 12.77 05:34:53.50 -02:51:41.3
206.59023 -18.30988 galactic Ori Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3216840069872616704 | 05:34:52.19 -02:51:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.394+/-0.029 (G)
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 23.2631* 05 34 53.50 -02 51 41.3 12.8 U Ori 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 3216840069872616704,2461032.7631,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3216840069872616704 20251223.2631 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:53.50 -02:51:41.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 12.28 05:21:02.83 +02:30:51.2
199.86412 -18.76293 galactic Ori Second-epoch detections are separated by 0.5" and 8.4 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 3234572138709057792 | 05:21:03.93 +02:31:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949AnHar.112....1C HD 287712 J-Ks=0.408+/-0.032 (G)
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 23.2631* 05 21 02.83 +02 30 51.2 12.3 U Ori 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 3234572138709057792,2461032.7631,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3234572138709057792 20251223.2631 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:02.83 +02:30:51.2 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 11.68 05:04:18.31 -03:00:52.1
202.85752 -25.11693 galactic Ori Second-epoch detections are separated by 0.8" and 8.3 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 | Large-amplitude variable Gaia DR2 3213232370360096512 | 05:04:19.43 -03:00:57.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G0 1949AnHar.112....1C HD 293765 J-Ks=0.235+/-0.031 (F)
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 23.2631* 05 04 18.31 -03 00 52.1 11.7 U Ori 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
Large-amplitude variable Gaia DR2 3213232370360096512,2461032.7631,11.68,0.05,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
Large-amplitude variable Gaia DR2 3213232370360096512 20251223.2631 11.68CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:04:18.31 -03:00:52.1 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 13.00 04:37:02.88 +02:07:37.4
194.01991 -28.37340 galactic Tau Second-epoch detections are separated by 0.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:37:02.88 +02:07:37.4 (user input) | T | P | (position from user input) J-Ks=0.568+/-0.034 (K)
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 23.2631* 04 37 02.88 +02 07 37.4 13.0 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,2461032.7631,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251223.2631 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:02.88 +02:07:37.4 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 37 09.25 -03 27 26.4 13.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3201877984361383168,2461032.7631,13.21,0.05,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 3201877984361383168 20251223.2631 13.21CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:09.25 -03:27:26.4 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 13.32 05:17:26.24 +01:55:11.4
199.93567 -19.84086 galactic Ori Second-epoch detections are separated by 0.4" and 8.4 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 3234433767746679680 | 05:17:27.13 +01:54:53.3 (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 23.2631* 05 17 26.24 +01 55 11.4 13.3 U Ori 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 3234433767746679680,2461032.7631,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3234433767746679680 20251223.2631 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:26.24 +01:55:11.4 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 13.93 05:13:13.09 -05:18:04.2
206.22806 -24.22967 galactic Ori Second-epoch detections are separated by 2.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3208775220802363392 | 05:13:12.12 -05:17:26.7 (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 23.2631* 05 13 13.09 -05 18 04.2 13.9 U Ori 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 3208775220802363392,2461032.7631,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3208775220802363392 20251223.2631 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:13.09 -05:18:04.2 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 37 14.20 -06 06 10.0 13.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461032.7631,13.94,0.05,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 20251223.2631 13.94CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:14.20 -06:06:10.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 13.97 04:37:07.72 -02:31:22.2
198.59258 -30.78464 galactic Eri Second-epoch detections are separated by 2.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:37:07.72 -02:31:22.2 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.037 (G)
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 23.2631* 04 37 07.72 -02 31 22.2 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,2461032.7631,13.97,0.05,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 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:07.72 -02:31:22.2 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 36 05.20 -06 29 31.6 14.1 U Ori 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
AW Ori,2461032.7631,14.13,0.05,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
AW Ori 20251223.2631 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:05.20 -06:29:31.6 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 17 51.69 +01 44 49.8 14.2 U Ori 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,2461032.7631,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251223.2631 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:51.69 +01:44:49.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.12 04:37:03.38 +01:45:13.3
194.37937 -28.57229 galactic Tau Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J069.2643+01.7560 | 04:37:03.38 +01:45:13.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
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 23.2631* 04 37 03.38 +01 45 13.3 14.1 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
ATO J069.2643+01.7560,2461032.7631,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J069.2643+01.7560 20251223.2631 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:03.38 +01:45:13.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 26 39.93 -07 04 32.9 14.3 U Ori 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
CSS_J052639.7-070432,2461032.7631,14.34,0.05,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
CSS_J052639.7-070432 20251223.2631 14.34CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:39.93 -07:04:32.9 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.29 05:15:23.36 +02:49:22.1
198.83243 -19.83227 galactic Ori Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:15:23.36 +02:49:22.1 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.034 (G)
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 23.2631* 05 15 23.36 +02 49 22.1 14.3 U Ori 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,2461032.7631,14.29,0.05,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 20251223.2631 14.29CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:23.36 +02:49:22.1 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.21 04:48:14.83 +01:46:15.9
196.03139 -26.19137 galactic Ori Second-epoch detections are separated by 1.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3232502544290811008 | 04:48:14.34 +01:46:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.377+/-0.042 (G)
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 23.2631* 04 48 14.83 +01 46 15.9 14.2 U Ori 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 3232502544290811008,2461032.7631,14.21,0.05,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 3232502544290811008 20251223.2631 14.21CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:48:14.83 +01:46:15.9 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.41 05:32:22.10 +03:10:22.2
200.72713 -15.97971 galactic Ori Second-epoch detections are separated by 1.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3223988338563860352 | 05:32:24.24 +03:10:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
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 23.2631* 05 32 22.10 +03 10 22.2 14.4 U Ori 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 3223988338563860352,2461032.7631,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3223988338563860352 20251223.2631 14.41CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:22.10 +03:10:22.2 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.29 05:29:48.81 -02:03:40.3
205.21766 -19.05729 galactic Ori Second-epoch detections are separated by 1.1" and 8.4 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 3217098665561622784 | 05:29:50.38 -02:03:06.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 290545
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 23.2631* 05 29 48.81 -02 03 40.3 14.3 U Ori 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 3217098665561622784,2461032.7631,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3217098665561622784 20251223.2631 14.29CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:48.81 -02:03:40.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.30 05:11:24.68 -05:31:42.9
206.22257 -24.73357 galactic Ori Second-epoch detections are separated by 0.4" and 8.4 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 3211667593514874752 | 05:11:26.78 -05:31:51.6 (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 23.2631* 05 11 24.68 -05 31 42.9 14.3 U Ori 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 3211667593514874752,2461032.7631,14.30,0.05,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 3211667593514874752 20251223.2631 14.30CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:24.68 -05:31:42.9 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.35 04:54:00.08 -04:51:38.8
203.30241 -28.25613 galactic Eri Second-epoch detections are separated by 2.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:00.08 -04:51:38.8 (user input) | T | P | (position from user input) J-Ks=0.668+/-0.039 (K)
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 23.2631* 04 54 00.08 -04 51 38.8 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,2461032.7631,14.35,0.05,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 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:00.08 -04:51:38.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 34 18.20 -05 33 33.4 14.4 U Ori 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
V1427 Ori,2461032.7631,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1427 Ori 20251223.2631 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:18.20 -05:33:33.4 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.49 05:30:40.46 +00:49:42.5
202.65029 -17.49084 galactic Ori Second-epoch detections are separated by 2.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:30:40.46 +00:49:42.5 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.048 (G)
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 23.2631* 05 30 40.46 +00 49 42.5 14.5 U Ori 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,2461032.7631,14.49,0.05,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 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:40.46 +00:49:42.5 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 24 49.85 -06 30 08.1 14.5 U Ori 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 3208912767132365184,2461032.7631,14.47,0.05,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
Gaia DR3 3208912767132365184 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:49.85 -06:30:08.1 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.24 04:42:58.92 -05:42:33.1
202.66454 -31.07345 galactic Eri Second-epoch detections are separated by 0.7" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:42:58.92 -05:42:33.1 (user input) | T | P | (position from user input) J-Ks=0.523+/-0.035 (K)
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 23.2631* 04 42 58.92 -05 42 33.1 14.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461032.7631,14.24,0.05,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 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:58.92 -05:42:33.1 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 44 17.19 +02 26 13.5 14.4 U Ori 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,2461032.7631,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251223.2631 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:44:17.19 +02:26:13.5 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 34 54.14 -04 21 33.3 14.4 U Ori 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
V1225 Ori,2461032.7631,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1225 Ori 20251223.2631 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:54.14 -04:21:33.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 30 27.62 -05 00 19.2 14.4 U Ori 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,2461032.7631,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251223.2631 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:27.62 -05:00:19.2 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 58 35.84 -06 04 19.9 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,2461032.7631,14.30,0.05,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 20251223.2631 14.30CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:35.84 -06:04:19.9 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.45 05:37:18.91 -03:26:00.3
207.41847 -18.03813 galactic Ori Second-epoch detections are separated by 2.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:37:18.91 -03:26:00.3 (user input) | T | P | (position from user input) J-Ks=0.577+/-0.038 (K)
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 23.2631* 05 37 18.91 -03 26 00.3 14.4 U Ori 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,2461032.7631,14.45,0.05,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 20251223.2631 14.45CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:18.91 -03:26:00.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 41 40.94 -07 11 25.0 14.4 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
target,2461032.7631,14.36,0.05,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 20251223.2631 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:40.94 -07:11:25.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.45 04:55:42.92 -06:39:32.8
205.33839 -28.71836 galactic Eri Second-epoch detections are separated by 0.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:42.92 -06:39:32.8 (user input) | T | P | (position from user input) J-Ks=0.475+/-0.043 (K)
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 23.2631* 04 55 42.92 -06 39 32.8 14.4 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
target,2461032.7631,14.45,0.05,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 20251223.2631 14.45CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:42.92 -06:39:32.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 29 15.79 -06 54 21.1 14.4 U Ori 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,2461032.7631,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251223.2631 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:15.79 -06:54:21.1 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.46 05:30:02.79 -00:15:51.0
203.57759 -18.15355 galactic Ori Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:30:02.79 -00:15:51.0 (user input) | T | P | (position from user input) J-Ks=0.295+/-0.038 (F)
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 23.2631* 05 30 02.79 +00 15 51.0 14.5 U Ori 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,2461032.7631,14.46,0.05,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 20251223.2631 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:02.79 -00:15:51.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.44 04:48:13.59 -04:04:17.8
201.72696 -29.14203 galactic Eri Second-epoch detections are separated by 1.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3200856297541228672 | 04:48:11.34 -04:03:58.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.522+/-0.037 (K)
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 23.2631* 04 48 13.59 -04 04 17.8 14.4 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
Gaia DR3 3200856297541228672,2461032.7631,14.44,0.05,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 3200856297541228672 20251223.2631 14.44CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:48:13.59 -04:04:17.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 41 50.87 -06 10 52.8 14.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461032.7631,14.24,0.05,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 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:50.87 -06:10:52.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.36 04:52:49.42 -03:03:57.2
201.36073 -27.65092 galactic Ori Second-epoch detections are separated by 0.7" and 8.3 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 3225033256862772736 | 04:52:48.66 -03:03:24.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
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 23.2631* 04 52 49.42 -03 03 57.2 14.4 U Ori 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 3225033256862772736,2461032.7631,14.36,0.05,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 3225033256862772736 20251223.2631 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:52:49.42 -03:03:57.2 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 40 27.40 +00 49 56.7 14.4 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
Gaia DR3 3230894272313460096,2461032.7631,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3230894272313460096 20251223.2631 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:40:27.40 +00:49:56.7 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 36 03.44 +00 45 45.0 14.5 U Ori 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,2461032.7631,14.49,0.05,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 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:03.44 +00:45:45.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.44 05:35:39.36 -01:47:40.7
205.69185 -17.64325 galactic Ori Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:35:39.36 -01:47:40.7 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5)
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 23.2631* 05 35 39.36 -01 47 40.7 14.4 U Ori 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,2461032.7631,14.44,0.05,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 20251223.2631 14.44CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:39.36 -01:47:40.7 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.35 05:22:47.58 -07:05:30.4
209.14632 -22.91985 galactic Ori Second-epoch detections are separated by 1.5" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3207353281687096064 | 05:22:46.74 -07:06:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.619+/-0.040 (K)
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 23.2631* 05 22 47.58 -07 05 30.4 14.3 U Ori 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 3207353281687096064,2461032.7631,14.35,0.05,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
Gaia DR3 3207353281687096064 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:47.58 -07:05:30.4 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 29 32.76 -06 32 03.5 14.4 U Ori 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,2461032.7631,14.45,0.05,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 20251223.2631 14.45CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:32.76 -06:32:03.5 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.21 04:42:59.41 -00:51:12.8
197.79478 -28.67467 galactic Eri Second-epoch detections are separated by 1.0" and 8.4 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 | ATO J070.7442-00.8479 | 04:42:59.41 -00:51:12.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.420+/-0.040 (G)
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 23.2631* 04 42 59.41 +00 51 12.8 14.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J070.7442-00.8479,2461032.7631,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J070.7442-00.8479 20251223.2631 14.21CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:59.41 -00:51:12.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.47 05:10:42.04 -05:24:17.9
206.01203 -24.83367 galactic Eri Second-epoch detections are separated by 2.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:10:42.04 -05:24:17.9 (user input) | T | P | (position from user input) J-Ks=0.479+/-0.037 (K)
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 23.2631* 05 10 42.04 -05 24 17.9 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,2461032.7631,14.47,0.05,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 20251223.2631 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:10:42.04 -05:24:17.9 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 36 01.57 -04 50 11.0 14.5 U Ori 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 3209561925670914816,2461032.7631,14.46,0.05,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 3209561925670914816 20251223.2631 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:01.57 -04:50:11.0 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 42 20.05 -06 16 52.3 14.4 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
target,2461032.7631,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251223.2631 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:20.05 -06:16:52.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 46 46.40 -04 56 41.2 14.4 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
target,2461032.7631,14.45,0.05,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 20251223.2631 14.45CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:46.40 -04:56:41.2 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.41 04:46:57.77 +00:43:46.2
196.83866 -27.00803 galactic Ori Second-epoch detections are separated by 2.4" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:46:57.77 +00:43:46.2 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.046 (G)
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 23.2631* 04 46 57.77 +00 43 46.2 14.4 U Ori 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,2461032.7631,14.41,0.05,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 20251223.2631 14.41CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:57.77 +00:43:46.2 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.50 04:57:21.52 -05:49:45.7
204.71678 -27.97272 galactic Eri Second-epoch detections are separated by 2.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.3370-05.8384 | 04:57:20.89 -05:50:18.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 23.2631* 04 57 21.52 -05 49 45.7 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
ATO J074.3370-05.8384,2461032.7631,14.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.3370-05.8384 20251223.2631 14.50CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:21.52 -05:49:45.7 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 04 43 54.90 -02 18 14.1 14.4 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
target,2461032.7631,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251223.2631 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:43:54.90 -02:18:14.1 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.45 04:41:51.63 +01:28:17.1
195.37521 -27.70630 galactic Tau Second-epoch detections are separated by 0.2" and 8.4 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 3231202822764439552 | 04:41:52.89 +01:27:43.9 (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 23.2631* 04 41 51.63 +01 28 17.1 14.4 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
Gaia DR3 3231202822764439552,2461032.7631,14.45,0.05,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 3231202822764439552 20251223.2631 14.45CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:51.63 +01:28:17.1 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.41 04:39:48.93 +02:55:40.3
193.67917 -27.35935 galactic Tau Second-epoch detections are separated by 2.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J069.9475+02.9217 | 04:39:48.93 +02:55:40.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.593+/-0.041 (K)
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 23.2631* 04 39 48.93 +02 55 40.3 14.4 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
ATO J069.9475+02.9217,2461032.7631,14.41,0.05,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
ATO J069.9475+02.9217 20251223.2631 14.41CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:48.93 +02:55:40.3 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.48 04:46:57.09 -06:01:09.7
203.52471 -30.34969 galactic Eri Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3187985178204980224 | 04:46:59.09 -06:01:37.3 (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 23.2631* 04 46 57.09 -06 01 09.7 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
Gaia DR3 3187985178204980224,2461032.7631,14.48,0.05,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
Gaia DR3 3187985178204980224 20251223.2631 14.48CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:57.09 -06:01:09.7 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 23.2631 2461032.7631 14.48 04:43:09.75 -01:41:37.8
198.64598 -29.06492 galactic Eri Second-epoch detections are separated by 1.5" and 8.3 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 3229133095204560128 | 04:43:09.12 -01:42:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5)
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 23.2631* 04 43 09.75 -01 41 37.8 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
Gaia DR3 3229133095204560128,2461032.7631,14.48,0.05,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
Gaia DR3 3229133095204560128 20251223.2631 14.48CV 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:43:09.75 -01:41:37.8 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_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 23.2631* 05 11 34.05 +00 19 06.6 13.1 U Ori 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
ASASSN-V J051133.87+001905.8,2461032.7631,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051133.87+001905.8 20251223.2631 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:34.05 +00:19:06.6 ;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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20_00sec_-14_90C_LIGHT_0302_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png animation_v2.gif
Processing complete!
Total number of candidates identified: 81
Processing log:
Images processed 4
Images used for photometry 4
Ref. image: 2461028.75433760 19.12.2025 06:06:04.769 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits
First image: 2461028.75433760 19.12.2025 06:06:04.769 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits
Last image: 2461032.76342100 23.12.2025 06:19:09.574 /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 20
Estimated ref. image limiting mag.: -10.74
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: 69 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): 14275
Objects passed selection criteria: 14266
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: 13477
Average stars matched: 12623 (93.6633 %)
Memory usage VmPeak: 97668 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 Thu Dec 25 21:43:35 -00 2025
Host name: tau
############################################################
Images processed 4
Images used for photometry 4
Ref. image: 2461028.75433760 19.12.2025 06:06:04.769 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits
First image: 2461028.75433760 19.12.2025 06:06:04.769 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits
Last image: 2461032.76342100 23.12.2025 06:19:09.574 /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 328
Estimated ref. image limiting mag.: -7.94
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: 167 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): 86428
Objects passed selection criteria: 86229
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: 82905.8
Average stars matched: 78076.2 (94.1747 %)
Memory usage VmPeak: 1026872 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 Thu Dec 25 21:48:59 -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:
Ori-05-Q1b1x1
#######################################
########### Starting Ori-05-Q1b1x1 ###########
Processing Ori-05-Q1b1x1
server tau has sufficient free disk space available: 649510 MB at /mnt/usb2/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 649510 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits
REFERENCE_EPOCH__SECOND_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png' -> 'transient_report/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits_preview.png'
Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
renamed 'Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png' -> 'transient_report/Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits_preview.png'
Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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= 843.5978
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 821.3376
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1204.3114
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 901.9704
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1203.5351
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 903.0761
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.42759
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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= '2025-12-23T00:18:20.0158278' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2025-12-23T06:18:20.0158278' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61032.262731655 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2025-12-23T06:18:29.9166157' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61032.2628462501 / 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 = 77.1401139334833 / [deg] RA of telescope" status=0
Record 32: "DEC = -1.9995371353795 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 53.6327777777778 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 192.344444444444 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.24116472019208 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / 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 = 'Ori-05' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '05 08 34' / [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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/d_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits :)
Spent 0.421752 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2025-12-22.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/d_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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= '2025-12-23T00:19:09.5744584' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2025-12-23T06:19:09.5744584' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61032.2633052547 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2025-12-23T06:19:19.4749061' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61032.2634198382 / 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 = 77.1401139152424 / [deg] RA of telescope" status=0
Record 32: "DEC = -1.99953712070593 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 53.595 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 192.690833333333 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.24176625603901 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / 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 = 'Ori-05' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '05 08 34' / [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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/d_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits :)
Spent 0.423998 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2025-12-22.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/d_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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: 2461032.76284740
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits exists and is non-empty
Saving wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits to local_wcs_cache/
'wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits' -> 'local_wcs_cache/wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits'
wcs_Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits exists and is non-empty
Saving wcs_Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits to local_wcs_cache/
'wcs_Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits' -> 'local_wcs_cache/wcs_Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits'
wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits exists and is non-empty
Saving wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits to local_wcs_cache/
'wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits' -> 'local_wcs_cache/wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits'
wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits exists and is non-empty
Saving wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits to local_wcs_cache/
'wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits' -> 'local_wcs_cache/wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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 05:08:36.918 -02:00:42.61
Second-epoch image center 05:08:15.374 -01:59:01.07
Angular distance between the image centers 0.09 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 05:08:36.918 -02:00:42.61
Second-epoch image center 05:08:13.434 -01:59:41.99
Angular distance between the image centers 0.10 deg.
###################################
Running solve_plate_with_UCAC5
Calibrating the magnitude scale
Found non-empty wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits and wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits and wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits.cat
Found non-empty wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits and wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits.cat
The reference image (wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits) and catalog (wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits.cat) found
'wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.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 7714 out of 12237 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.769614
a=0.000000 b=1.000000 c=22.769614
From vast_summary.log: estimated ref. image limiting mag.: -10.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.03
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.03
____ 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 19 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits
2.0 pix Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits
2.0 pix fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
2.0 pix fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits
All-image limiting magnitude estimate: 12.0 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_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits'
'wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits'
Preparing the HTML report for the field Ori-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20734.dat to exclusion_list_local.txt
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Considering the candidate 20657_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
The candidate 20657_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302 did not pass the final checks
**** FOUND 05:24:34.61 -02:22:37.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 20671_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20671_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20671_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20671_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20671_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20704_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20704_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20704_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20704_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20704_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20709_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20709_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20709_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20709_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20709_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20711_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20711_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20711_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20711_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20711_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20713_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20713_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20713_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20713_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20713_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20714_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20714_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20714_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20714_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20714_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20716_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20716_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20716_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20716_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20716_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20717_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20717_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20717_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20717_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20717_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20721_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20721_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20721_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20721_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20721_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20722_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20722_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20722_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20722_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20722_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20723_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20723_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20723_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20723_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20723_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20725_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20725_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20725_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20725_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20725_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20726_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20726_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20726_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20726_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20726_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 20727_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20727_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20727_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20727_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20727_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20728_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20728_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20728_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20728_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20728_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20729_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20729_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20729_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20729_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20729_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20733_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20733_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20733_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20733_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20733_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20734_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 20734_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/20734_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/20734_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/20734_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
Prepared the HTML report for the field Ori-05-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 ####
05:03:58.50 -03:30:13.1
05:01:21.54 -00:43:16.5
05:26:08.97 +00:49:41.7
05:18:18.85 +02:23:51.5
05:11:57.50 -01:32:24.6
05:17:15.56 -01:58:34.8
05:35:31.99 -05:09:28.0
05:08:10.90 -02:40:18.8
05:13:09.44 -02:03:25.9
05:34:42.04 -03:41:56.8
05:25:53.15 -00:11:55.4
05:12:36.45 -03:15:06.5
05:27:31.65 -05:05:21.0
05:16:19.35 -01:52:14.0
05:06:26.77 -05:54:18.4
05:35:46.71 -05:17:57.2
05:13:25.03 +02:38:35.3
05:12:13.59 -01:50:31.3
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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits
Creating symlink local_wcs_cache/wcs_Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Creating symlink local_wcs_cache/exclusion_list_bbsc.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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits exists and is non-empty
wcs_Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits exists and is non-empty
wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits exists and is non-empty
wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.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 05:08:36.918 -02:00:42.61
Second-epoch image center 05:08:15.374 -01:59:01.07
Angular distance between the image centers 0.09 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 05:08:36.918 -02:00:42.61
Second-epoch image center 05:08:13.434 -01:59:41.99
Angular distance between the image centers 0.10 deg.
###################################
Running solve_plate_with_UCAC5
Calibrating the magnitude scale
Found non-empty wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits and wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.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_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits and wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits.cat
Found non-empty wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits and wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits.cat
The reference image (wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits) and catalog (wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits.cat) found
'wcs_Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.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 8139 out of 78439 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.629255
a=0.000000 b=1.000000 c=22.629255
From vast_summary.log: estimated ref. image limiting mag.: -7.94
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 71 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits
1.8 pix Ori-05-Q1b1x1_2025-12-19_00-06-35_20.00sec_-15.00C_LIGHT_0260.fits
1.9 pix fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
1.9 pix fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits
All-image limiting magnitude estimate: 14.5 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_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits'
'wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-25_CI_Ori-05-Q1b1x1_213552_TTUQ1b1x1_19077_Zrqxwrut/wcs_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.fits'
Preparing the HTML report for the field Ori-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 131: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 131: echo: write error: Broken pipe
Adding exclusion_list_local.txt__out25455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95876.dat to exclusion_list_local.txt
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Considering the candidate 94944_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94944_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94944_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94944_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94944_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94952_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94952_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94952_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94952_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94952_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94953_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94953_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94953_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94953_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94953_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94961_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94961_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94961_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94961_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94961_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94964_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94964_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94964_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94964_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94964_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94974_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94974_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94974_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94974_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94974_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94982_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94982_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94982_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94982_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94982_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94985_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94985_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94985_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94985_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94985_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94990_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94990_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94990_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94990_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94990_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94991_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94991_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94991_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94991_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94991_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94993_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94993_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94993_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94993_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94993_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94995_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94995_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94995_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94995_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94995_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 94997_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 94997_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/94997_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/94997_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/94997_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95025_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
The candidate 95025_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302 did not pass the final checks
**** FOUND 05:24:34.63 -02:22:37.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 95215_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95215_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95215_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95215_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95215_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95260_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95260_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95260_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95260_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95260_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95274_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95274_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95274_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95274_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95274_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95317_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
The candidate 95317_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 95405_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95405_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95405_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95405_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95405_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95408_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95408_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95408_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95408_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95408_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95442_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95442_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95442_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95442_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95442_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95468_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
The candidate 95468_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302 did not pass the final checks
**** FOUND 05:38:33.01 -02:35:37.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 95487_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95487_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95487_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95487_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95487_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95503_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95503_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95503_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95503_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95503_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95506_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95506_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95506_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95506_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95506_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95514_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
The candidate 95514_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302 did not pass the final checks
**** FOUND 05:26:49.12 +03:03:43.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 95516_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95516_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95516_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95516_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95516_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95528_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95528_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95528_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95528_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95528_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95532_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95532_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95532_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95532_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95532_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95535_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95535_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95535_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95535_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95535_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95536_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95536_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95536_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95536_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95536_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95538_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
The candidate 95538_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302 did not pass the final checks
**** FOUND 05:31:46.65 -00:19:04.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 95551_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95551_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95551_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95551_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95551_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95554_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95554_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95554_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95554_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95554_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95563_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95563_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95563_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95563_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95563_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95564_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
The candidate 95564_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302 did not pass the final checks
**** FOUND 05:24:41.19 +01:54:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95566_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95566_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95566_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95566_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95566_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95577_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95577_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95577_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95577_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95577_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95578_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95578_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95578_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95578_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95578_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95580_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95580_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95580_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95580_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95580_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95586_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95586_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95586_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95586_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95586_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95588_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95588_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95588_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95588_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95588_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95589_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95589_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95589_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95589_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95589_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95590_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
The candidate 95590_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302 did not pass the final checks
**** FOUND 05:17:33.99 -06:48:21.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 95595_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95595_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95595_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95595_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95595_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95599_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95599_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95599_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95599_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95599_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95609_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95609_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95609_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95609_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95609_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95612_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95612_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95612_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95612_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95612_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95617_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95617_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95617_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95617_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95617_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95619_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95619_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95619_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95619_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95619_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95620_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95620_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95620_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95620_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95620_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95621_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95621_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95621_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95621_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95621_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95622_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95622_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95622_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95622_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95622_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95627_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95627_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95627_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95627_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95627_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95647_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95647_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95647_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95647_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95647_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95650_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Preparing report for the candidate 95650_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
Successfully moved Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.png to transient_report/95650_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_reference.png
The output file transient_report/Ori-05-Q1b1x1_2025-12-19_00-06-04_20.00sec_-15.00C_LIGHT_0259.fits_preview.png already exist
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.png to transient_report/95650_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery1.png
Successfully moved fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302.png to transient_report/95650_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302_discovery2.png
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Considering the candidate 95653_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302
The candidate 95653_fd_Ori-05-Q1b1x1_2025-12-23_00-19-09_20.00sec_-14.90C_LIGHT_0302 did not pass the final checks