This analysis is done by the script util/transients/transient_factory_test31.sh /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 20 42.41 +50 30 39.8 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:20:42.41 +50:30:39.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 08 05.75 +45 51 21.7 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 11.89CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:08:05.75 +45:51:21.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 09 19.22 +46 24 05.3 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.98,0.05,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
target 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:09:19.22 +46:24:05.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.04 23:25:21.53 +49:41:02.2
108.94832 -10.83629 galactic And Second-epoch detections are separated by 8.5" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J351.3632+49.6943 | 23:25:25.43 +49:41:10.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 27.0772* 23 25 21.53 +49 41 02.2 12.0 U And 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 J351.3632+49.6943,2461036.5772,12.04,0.05,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
ATO J351.3632+49.6943 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:25:21.53 +49:41:02.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 21 40.43 +46 18 43.3 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.08CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:21:40.43 +46:18:43.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.07 00:22:01.68 +45:29:22.5
117.54675 -17.07443 galactic And Second-epoch detections are separated by 0.3" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391841003266975488 | 00:21:58.78 +45:29:22.0 (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 27.0772* 00 22 01.68 +45 29 22.5 12.1 U And 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 391841003266975488,2461036.5772,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 391841003266975488 20251227.0772 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:22:01.68 +45:29:22.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 14 11.12 +45 24 09.7 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.10CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:14:11.12 +45:24:09.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.12 00:06:41.67 +45:19:58.7
114.74093 -16.82598 galactic And Second-epoch detections are separated by 2.1" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 386452120682910976 | 00:06:43.70 +45:20:30.8 (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 27.0772* 00 06 41.67 +45 19 58.7 12.1 U And 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 386452120682910976,2461036.5772,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 386452120682910976 20251227.0772 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:06:41.67 +45:19:58.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 07 32.84 +47 41 55.2 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.14,0.05,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
target 20251227.0772 12.14CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:07:32.84 +47:41:55.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 39 19.92 +50 59 06.8 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:39:19.92 +50:59:06.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 35 53.53 +48 58 06.5 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:53.53 +48:58:06.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 29 48.42 +50 12 04.5 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.21,0.05,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
target 20251227.0772 12.21CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:48.42 +50:12:04.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.22 00:17:07.69 +48:33:13.7
117.09410 -13.92866 galactic Cas Second-epoch detections are separated by 5.5" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 392819740415954432 | 00:17:07.55 +48:33:52.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 17 07.69 +48 33 13.7 12.2 U Cas 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 392819740415954432,2461036.5772,12.22,0.05,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 392819740415954432 20251227.0772 12.22CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:17:07.69 +48:33:13.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 02 46.58 +46 47 49.5 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.26CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:02:46.58 +46:47:49.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.22 23:59:18.08 +45:47:25.5
113.51017 -16.12538 galactic And Second-epoch detections are separated by 1.4" and 1.7 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 1926323107483163904 | 23:59:13.79 +45:47:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 59 18.08 +45 47 25.5 12.2 U And 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 1926323107483163904,2461036.5772,12.22,0.05,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 1926323107483163904 20251227.0772 12.22CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:59:18.08 +45:47:25.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 06 50.69 +47 01 28.3 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.22CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:06:50.69 +47:01:28.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 15 45.58 +46 23 39.1 12.2 U And 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 392127116808474368,2461036.5772,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 392127116808474368 20251227.0772 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:15:45.58 +46:23:39.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 11 32.13 +46 42 40.0 12.2 U And 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
ZTF J001133.71+464232.5,2461036.5772,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J001133.71+464232.5 20251227.0772 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:11:32.13 +46:42:40.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 02 57.34 +47 55 08.5 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.26CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:02:57.34 +47:55:08.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 16 13.85 +49 58 20.8 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:13.85 +49:58:20.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 56 43.00 +45 32 21.8 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.27CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:56:43.00 +45:32:21.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 47 04.45 +43 03 37.0 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.27CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:47:04.45 +43:03:37.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 33 56.05 +47 42 30.3 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:33:56.05 +47:42:30.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 29 53.87 +46 38 27.6 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.98,0.05,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
target 20251227.0772 12.98CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:29:53.87 +46:38:27.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.79 23:19:37.11 +49:33:15.0
108.01408 -10.63948 galactic And Second-epoch detections are separated by 6.7" and 1.5 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 | 23:19:37.11 +49:33:15.0 (user input) | T | P | (position from user input) J-Ks=0.510+/-0.062 (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 27.0772* 23 19 37.11 +49 33 15.0 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.79,0.05,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
target 20251227.0772 12.79CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:19:37.11 +49:33:15.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.77 23:37:21.55 +45:50:15.4
109.68040 -15.11943 galactic And Second-epoch detections are separated by 5.0" and 1.9 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 J354.3386+45.8351 | 23:37:21.55 +45:50:15.4 (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 27.0772* 23 37 21.55 +45 50 15.4 12.8 U And 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 J354.3386+45.8351,2461036.5772,12.77,0.05,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
ATO J354.3386+45.8351 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:37:21.55 +45:50:15.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 47 23.48 +50 23 29.1 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.80CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:47:23.48 +50:23:29.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 56 16.49 +50 06 50.6 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.80CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:56:16.49 +50:06:50.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 32 08.19 +45 32 49.8 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:32:08.19 +45:32:49.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 29 24.06 +49 00 07.8 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.70CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:29:24.06 +49:00:07.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 48 50.84 +48 52 52.0 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:48:50.84 +48:52:52.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 17 03.89 +47 22 32.0 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:17:03.89 +47:22:32.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 33 30.84 +47 47 42.9 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:33:30.84 +47:47:42.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.55 23:27:05.66 +45:37:42.4
107.85161 -14.75918 galactic And Second-epoch detections are separated by 3.7" and 1.5 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 J351.7712+45.6280 | 23:27:05.66 +45:37:42.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) 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 27.0772* 23 27 05.66 +45 37 42.4 12.6 U And 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 J351.7712+45.6280,2461036.5772,12.55,0.05,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 J351.7712+45.6280 20251227.0772 12.55CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:27:05.66 +45:37:42.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 25 45.61 +50 15 15.7 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.44,0.05,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 20251227.0772 12.44CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:25:45.61 +50:15:15.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 36 38.54 +44 01 25.7 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.49CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:36:38.54 +44:01:25.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 06 49.66 +49 57 35.8 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:06:49.66 +49:57:35.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 31 24.40 +48 27 32.7 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:31:24.40 +48:27:32.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 37 50.52 +45 49 18.9 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:37:50.52 +45:49:18.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 47 37.25 +49 42 55.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:47:37.25 +49:42:55.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 17 11.97 +49 03 03.1 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:17:11.97 +49:03:03.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.10 23:24:41.66 +46:40:40.8
107.81002 -13.63106 galactic And Second-epoch detections are separated by 4.8" and 2.3 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 1938616575196013696 | 23:24:40.10 +46:41:02.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1952IzKry...9...82G BD+45 4215
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 24 41.66 +46 40 40.8 12.1 U And 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 1938616575196013696,2461036.5772,12.10,0.05,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 1938616575196013696 20251227.0772 12.10CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:24:41.66 +46:40:40.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 44 02.14 +49 47 21.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:44:02.14 +49:47:21.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.03 00:24:57.86 +49:32:11.3
118.52736 -13.10874 galactic Cas Second-epoch detections are separated by 6.3" and 1.2 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 J006.2182+49.5363 | 00:24:56.50 +49:32:25.7 (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 27.0772* 00 24 57.86 +49 32 11.3 12.0 U Cas 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 J006.2182+49.5363,2461036.5772,12.03,0.05,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
ATO J006.2182+49.5363 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:24:57.86 +49:32:11.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 28 28.65 +48 37 00.6 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:28.65 +48:37:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 34 22.02 +44 47 17.7 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:34:22.02 +44:47:17.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 36 18.57 +48 24 08.8 11.9 U And 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
ZTF J233617.73+482429.3,2461036.5772,11.89,0.05,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
ZTF J233617.73+482429.3 20251227.0772 11.89CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:36:18.57 +48:24:08.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 38 28.02 +44 44 56.4 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:38:28.02 +44:44:56.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 27 02.23 +47 40 58.7 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:27:02.23 +47:40:58.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 22 41.61 +44 55 44.6 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:41.61 +44:55:44.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 38 20.17 +47 45 41.8 11.7 U Cas 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 390112639709334528,2461036.5772,11.66,0.05,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 390112639709334528 20251227.0772 11.66CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:20.17 +47:45:41.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 16 52.22 +47 18 27.6 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.46,0.05,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 20251227.0772 11.46CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:52.22 +47:18:27.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 11.07 23:53:07.51 +48:27:31.7
113.05618 -13.29160 galactic And Second-epoch detections are separated by 5.8" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J358.2974+48.4579 | 23:53:07.51 +48:27:31.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.282+/- (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 53 07.51 +48 27 31.7 11.1 U And 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 J358.2974+48.4579,2461036.5772,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.2974+48.4579 20251227.0772 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:53:07.51 +48:27:31.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 21 15.01 +44 58 34.3 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 11.04CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:15.01 +44:58:34.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 32 19.97 +45 20 06.3 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:32:19.97 +45:20:06.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 30 24.10 +47 05 22.1 10.9 U And 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 1938689830157855616,2461036.5772,10.88,0.05,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 1938689830157855616 20251227.0772 10.88CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:30:24.10 +47:05:22.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 34 04.87 +41 58 35.4 9.8 U And 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 1923840066630929792,2461036.5772,9.79,0.05,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 1923840066630929792 20251227.0772 9.79CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:34:04.87 +41:58:35.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 37 47.79 +44 03 50.7 9.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:37:47.79 +44:03:50.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 31 29.03 +48 47 32.4 11.1 U And 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 1942079555788092416,2461036.5772,11.10,0.05,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 1942079555788092416 20251227.0772 11.10CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:31:29.03 +48:47:32.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 32 35.28 +45 14 50.3 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.21,0.05,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
target 20251227.0772 11.21CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:32:35.28 +45:14:50.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 35 28.58 +48 35 51.3 11.2 U And 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 1943325160725481344,2461036.5772,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943325160725481344 20251227.0772 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:35:28.58 +48:35:51.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 21 20.66 +43 36 39.5 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:20.66 +43:36:39.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 11.61 00:26:51.47 +44:45:21.4
118.35027 -17.89703 galactic And Second-epoch detections are separated by 8.7" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 varaible 388790064659106432 | 00:26:47.71 +44:45:38.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: G8 (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 27.0772* 00 26 51.47 +44 45 21.4 11.6 U And 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 varaible 388790064659106432,2461036.5772,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 varaible 388790064659106432 20251227.0772 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:51.47 +44:45:21.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 11.60 00:30:49.06 +47:31:23.1
119.32695 -15.20428 galactic Cas Second-epoch detections are separated by 4.3" and 1.6 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 | Large-amplitude variable Gaia DR2 390973759175121664 | 00:30:45.61 +47:31:46.6 (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: G2 1952IzKry...9...82G BD+46 95
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 30 49.06 +47 31 23.1 11.6 U Cas 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 390973759175121664,2461036.5772,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 390973759175121664 20251227.0772 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:49.06 +47:31:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 11.98 23:35:51.37 +48:16:32.2
110.16708 -12.71398 galactic And Second-epoch detections are separated by 4.9" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1940302568900888576 | 23:35:48.57 +48:16:00.3 (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 27.0772* 23 35 51.37 +48 16 32.2 12.0 U And 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 1940302568900888576,2461036.5772,11.98,0.05,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 1940302568900888576 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:35:51.37 +48:16:32.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 52 45.93 +49 59 59.1 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:52:45.93 +49:59:59.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 33 47.62 +45 31 37.2 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.00,0.05,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
target 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:33:47.62 +45:31:37.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 30 18.32 +48 41 22.0 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.02CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:30:18.32 +48:41:22.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 23 43.08 +49 53 54.4 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.30,0.05,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 20251227.0772 12.30CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:23:43.08 +49:53:54.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 35 52.23 +48 42 32.4 12.6 U And 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 1943335266786029568,2461036.5772,12.59,0.05,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 1943335266786029568 20251227.0772 12.59CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:35:52.23 +48:42:32.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 31 30.79 +45 54 12.0 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.36,0.05,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 20251227.0772 12.36CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:31:30.79 +45:54:12.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 19 36.76 +43 38 38.2 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:19:36.76 +43:38:38.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 27 14.55 +44 20 09.4 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:27:14.55 +44:20:09.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 33 22.22 +44 48 25.5 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:33:22.22 +44:48:25.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 21 51.76 +48 50 40.6 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:51.76 +48:50:40.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.67 23:22:24.01 +49:16:35.2
108.34737 -11.05740 galactic And Second-epoch detections are separated by 8.6" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.5856+49.2818 | 23:22:24.01 +49:16:35.2 (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 27.0772* 23 22 24.01 +49 16 35.2 12.7 U And 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 J350.5856+49.2818,2461036.5772,12.67,0.05,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 J350.5856+49.2818 20251227.0772 12.67CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:24.01 +49:16:35.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 38 32.80 +45 54 23.9 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.70CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:38:32.80 +45:54:23.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.54 23:33:58.69 +45:30:35.5
108.99481 -15.25534 galactic And Second-epoch detections are separated by 6.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.4931+45.5215 | 23:33:58.69 +45:30:35.5 (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 27.0772* 23 33 58.69 +45 30 35.5 12.5 U And 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 J353.4931+45.5215,2461036.5772,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.4931+45.5215 20251227.0772 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:33:58.69 +45:30:35.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 30 36.94 +48 36 35.5 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:30:36.94 +48:36:35.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 18 31.25 +44 35 18.7 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:31.25 +44:35:18.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 28 40.70 +49 14 25.8 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:28:40.70 +49:14:25.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.82 23:18:20.50 +47:18:58.4
106.99684 -12.65460 galactic And Second-epoch detections are separated by 4.6" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:18:20.50 +47:18:58.4 (user input) | T | P | (position from user input) 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 27.0772* 23 18 20.50 +47 18 58.4 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:20.50 +47:18:58.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 22 26.96 +45 08 44.9 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.73CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:26.96 +45:08:44.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 27 02.91 +47 41 40.4 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.91,0.05,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
target 20251227.0772 12.91CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:27:02.91 +47:41:40.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 18 38.56 +45 19 24.5 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.79,0.05,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
target 20251227.0772 12.79CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:38.56 +45:19:24.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 27 07.16 +45 16 54.5 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.77,0.05,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
target 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:27:07.16 +45:16:54.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.67 23:22:10.38 +49:31:25.1
108.39858 -10.81256 galactic And Second-epoch detections are separated by 7.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.5238+49.5235 | 23:22:08.69 +49:31:59.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG+49 2092
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 22 10.38 +49 31 25.1 12.7 U And 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 J350.5238+49.5235,2461036.5772,12.67,0.05,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 J350.5238+49.5235 20251227.0772 12.67CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:10.38 +49:31:25.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.74 23:26:37.49 +48:33:58.2
108.77062 -11.95967 galactic And Second-epoch detections are separated by 4.4" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J351.6695+48.5592 | 23:26:41.84 +48:33:57.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 27.0772* 23 26 37.49 +48 33 58.2 12.7 U And 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 J351.6695+48.5592,2461036.5772,12.74,0.05,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 J351.6695+48.5592 20251227.0772 12.74CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:37.49 +48:33:58.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 19 31.02 +50 13 43.9 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:19:31.02 +50:13:43.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 55 58.43 +46 25 34.2 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:55:58.43 +46:25:34.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 20 56.83 +48 53 16.2 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.79,0.05,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
target 20251227.0772 12.79CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:20:56.83 +48:53:16.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.88 23:17:54.28 +46:34:49.0
106.65231 -13.31375 galactic And Second-epoch detections are separated by 0.8" and 1.3 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 | target | 23:17:54.28 +46:34:49.0 (user input) | T | P | (position from user input) J-Ks=0.199+/-0.180 (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 27.0772* 23 17 54.28 +46 34 49.0 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.88CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:17:54.28 +46:34:49.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 09 03.73 +50 43 23.3 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.91,0.05,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
target 20251227.0772 12.91CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:09:03.73 +50:43:23.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 22 29.93 +48 47 24.6 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:29.93 +48:47:24.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.77 23:26:04.81 +49:12:03.5
108.89798 -11.33083 galactic And Second-epoch detections are separated by 7.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J351.5303+49.2038 | 23:26:04.81 +49:12:03.5 (user input) | MSINE (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 27.0772* 23 26 04.81 +49 12 03.5 12.8 U And 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 J351.5303+49.2038,2461036.5772,12.77,0.05,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
ATO J351.5303+49.2038 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:04.81 +49:12:03.5 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 19 25.34 +46 38 15.6 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.74CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:19:25.34 +46:38:15.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 13.04 23:54:11.39 +48:47:21.3
113.30946 -13.00997 galactic Cas Second-epoch detections are separated by 3.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J358.5384+48.7790 | 23:54:11.39 +48:47:21.3 (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 27.0772* 23 54 11.39 +48 47 21.3 13.0 U Cas 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 J358.5384+48.7790,2461036.5772,13.04,0.05,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
ATO J358.5384+48.7790 20251227.0772 13.04CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:54:11.39 +48:47:21.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.75 23:16:32.41 +46:48:30.0
106.51417 -13.01599 galactic And Second-epoch detections are separated by 5.1" and 1.5 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 | HAT-161-0005921 | 23:16:30.84 +46:48:53.2 (Gaia DR3) | VAR (local) | 1.911469000000 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 16 32.41 +46 48 30.0 12.8 U And 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
HAT-161-0005921,2461036.5772,12.75,0.05,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
HAT-161-0005921 20251227.0772 12.75CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:32.41 +46:48:30.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 21 19.85 +46 04 51.9 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 13.04CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:19.85 +46:04:51.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 26 19.17 +49 26 59.3 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:19.17 +49:26:59.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 37 30.44 +47 27 31.2 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.03,0.05,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
target 20251227.0772 13.03CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:37:30.44 +47:27:31.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 29 54.59 +44 52 51.2 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:29:54.59 +44:52:51.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 43 06.34 +49 22 35.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:43:06.34 +49:22:35.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 16 16.30 +47 20 17.9 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:16.30 +47:20:17.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 20 34.93 +50 00 37.7 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.91,0.05,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
target 20251227.0772 12.91CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:20:34.93 +50:00:37.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 38 20.77 +48 16 01.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:20.77 +48:16:01.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 48 51.40 +50 28 00.9 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 13.02CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:48:51.40 +50:28:00.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 26 24.18 +45 01 16.8 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.73CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:24.18 +45:01:16.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 21 08.74 +44 32 12.0 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.80CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:08.74 +44:32:12.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 20 21.34 +46 12 38.1 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:20:21.34 +46:12:38.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 49 33.26 +49 51 24.4 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:49:33.26 +49:51:24.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 56 07.79 +47 00 02.7 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:56:07.79 +47:00:02.7 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 00 44.40 +50 42 15.6 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.88CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:00:44.40 +50:42:15.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 26 39.65 +50 09 41.3 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.97CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:39.65 +50:09:41.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 56 13.88 +47 19 04.0 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:56:13.88 +47:19:04.0 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 22 46.31 +50 55 44.3 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:46.31 +50:55:44.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.80 23:17:39.70 +47:26:22.3
106.93255 -12.49802 galactic And Second-epoch detections are separated by 1.2" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J349.4105+47.4375 | 23:17:39.70 +47:26:22.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F4 (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 27.0772* 23 17 39.70 +47 26 22.3 12.8 U And 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 J349.4105+47.4375,2461036.5772,12.80,0.05,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 J349.4105+47.4375 20251227.0772 12.80CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:17:39.70 +47:26:22.3 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 44 37.26 +50 13 05.9 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.88CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:44:37.26 +50:13:05.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 26 58.91 +50 08 45.1 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 13.01CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:58.91 +50:08:45.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 51 26.37 +50 51 24.1 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.91,0.05,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
target 20251227.0772 12.91CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:51:26.37 +50:51:24.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 13.11 23:45:53.75 +49:17:53.8
112.08388 -12.18800 galactic Cas Second-epoch detections are separated by 2.4" and 1.6 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 | ASASSN-V J234553.01+491823.0 | 23:45:53.01 +49:18:22.9 (Gaia DR3) | SR (local) | 2459059.75900 (local) | Gaia3var=VARIABLE 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 27.0772* 23 45 53.75 +49 17 53.8 13.1 U Cas 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 J234553.01+491823.0,2461036.5772,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J234553.01+491823.0 20251227.0772 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:45:53.75 +49:17:53.8 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 28 19.79 +49 59 09.5 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:28:19.79 +49:59:09.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.90 23:17:54.13 +47:32:15.2
107.00769 -12.42136 galactic And Second-epoch detections are separated by 3.0" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1941572573548528384 | 23:17:55.75 +47:32:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (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 27.0772* 23 17 54.13 +47 32 15.2 12.9 U And 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 1941572573548528384,2461036.5772,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1941572573548528384 20251227.0772 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:17:54.13 +47:32:15.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 25 17.56 +50 34 18.1 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.89CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:25:17.56 +50:34:18.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 27 09.97 +45 04 11.2 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.89CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:27:09.97 +45:04:11.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 18 09.74 +49 24 09.1 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:09.74 +49:24:09.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 17 59.18 +47 02 14.1 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:17:59.18 +47:02:14.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 36 08.14 +47 25 05.2 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.89CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:36:08.14 +47:25:05.2 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 00 37 55.63 +47 56 25.6 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:55.63 +47:56:25.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 21 31.10 +44 44 24.2 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:31.10 +44:44:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 12.96 23:41:55.15 +50:43:06.9
111.83718 -10.64952 galactic Cas Second-epoch detections are separated by 6.9" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.4874+50.7112 | 23:41:55.15 +50:43:06.9 (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 27.0772* 23 41 55.15 +50 43 06.9 13.0 U Cas 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 J355.4874+50.7112,2461036.5772,12.96,0.05,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
ATO J355.4874+50.7112 20251227.0772 12.96CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:41:55.15 +50:43:06.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 21 45.82 +49 52 41.4 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,12.91,0.05,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
target 20251227.0772 12.91CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:45.82 +49:52:41.4 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 31 49.15 +48 30 10.6 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:31:49.15 +48:30:10.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 13.07 23:29:39.38 +48:59:53.9
109.39618 -11.71217 galactic And Second-epoch detections are separated by 4.4" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.4195+49.0096 | 23:29:37.51 +49:00:25.6 (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 27.0772* 23 29 39.38 +48 59 53.9 13.1 U And 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 J352.4195+49.0096,2461036.5772,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.4195+49.0096 20251227.0772 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:29:39.38 +48:59:53.9 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 54 45.52 +49 34 54.6 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,13.14,0.05,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
target 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:54:45.52 +49:34:54.6 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2025 12 27.0772 2461036.5772 13.10 23:42:46.75 +46:51:36.1
110.90652 -14.40232 galactic And Second-epoch detections are separated by 8.4" and 1.7 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 1939232095549965184 | 23:42:49.97 +46:51:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G/K 1952IzKry...9...82G BD+46 4140
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 42 46.75 +46 51 36.1 13.1 U And 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 1939232095549965184,2461036.5772,13.10,0.05,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 1939232095549965184 20251227.0772 13.10CV 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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:42:46.75 +46:51:36.1 ;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_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20_00sec_-14_90C_LIGHT_0098_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2025 12 27.0772* 23 53 23.50 +50 08 37.1 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461036.5772,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20251227.0772 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/And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:53:23.50 +50:08:37.1 ;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_And-01-Q1b1x1_2025-12-18_22-16-22_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-01-Q1b1x1_2025-12-18_22-16-22_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-16-22_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-01-Q1b1x1_2025-12-18_22-16-22_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png resample_wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Processing complete!
Total number of candidates identified: 137
Processing log:
Images processed 4
Images used for photometry 4
Ref. image: 2461028.67780647 19.12.2025 04:15:52.479 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits
First image: 2461028.67780647 19.12.2025 04:15:52.479 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits
Last image: 2461036.57740700 27.12.2025 01:51:17.965 /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 27
Estimated ref. image limiting mag.: -10.52
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: 41 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): 23627
Objects passed selection criteria: 23619
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 22878.2
Average stars matched: 22334.5 (97.6233 %)
Memory usage VmPeak: 105836 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Thu Dec 25 11:45:33 -00 2025
VaST build number 1.0rc88-81-g00db519e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2025-12-25)
GNU bash, version 5.3.3(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Dec 27 01:59:51 -00 2025
Host name: tau
############################################################
Images processed 4
Images used for photometry 4
Ref. image: 2461028.67780647 19.12.2025 04:15:52.479 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits
First image: 2461028.67780647 19.12.2025 04:15:52.479 /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits
Last image: 2461036.57740700 27.12.2025 01:51:17.965 /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 313
Estimated ref. image limiting mag.: -7.81
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: 533 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): 160628
Objects passed selection criteria: 160219
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: 152731
Average stars matched: 148066 (96.9451 %)
Memory usage VmPeak: 1327588 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Thu Dec 25 11:45:33 -00 2025
VaST build number 1.0rc88-81-g00db519e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2025-12-25)
GNU bash, version 5.3.3(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Dec 27 02:22:08 -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:
And-01-Q1b1x1
#######################################
########### Starting And-01-Q1b1x1 ###########
Processing And-01-Q1b1x1
server tau has sufficient free disk space available: 609145 MB at /mnt/usb2/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 609145 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits
REFERENCE_EPOCH__SECOND_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png' -> 'transient_report/And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits_preview.png'
And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
renamed 'And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png' -> 'transient_report/And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits_preview.png'
And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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= 585.6551
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 750.1032
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1245.8099
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 805.4620
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1246.1108
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 806.1542
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.12721
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= -14.9 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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= '2025-12-26T19:50:42.0371489' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2025-12-27T01:50:42.0371489' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61036.0768754282 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2025-12-27T01:50:51.9370806' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61036.0769900116 / 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 = 359.997534913017 / [deg] RA of telescope" status=0
Record 32: "DEC = 45.9999196750289 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 69.6202777777778 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 313.79 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.0665554656415 / 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 = 'And-01' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '00 00 00' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+46 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/d_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits :)
Spent 0.437299 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2025-12-22.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/d_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -15.0 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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= '2025-12-26T19:51:17.9656005' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2025-12-27T01:51:17.9656005' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61036.0772912614 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2025-12-27T01:51:27.8667276' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61036.0774058565 / 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 = 359.997534960717 / [deg] RA of telescope" status=0
Record 32: "DEC = 45.9999196858745 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 69.53 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 313.641388888889 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.06718003006869 / 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 = 'And-01' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '00 00 00' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+46 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2025-12-22.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/d_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits :)
Spent 0.417560 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2025-12-22.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/d_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Dark frame used to calibrate the second-epoch images:
Flat field used to calibrate the second-epoch images:
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461036.57699117
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits exists and is non-empty
Saving wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits to local_wcs_cache/
'wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits' -> 'local_wcs_cache/wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits'
wcs_And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
Saving wcs_And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits to local_wcs_cache/
'wcs_And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits' -> 'local_wcs_cache/wcs_And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits'
wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
Saving wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits to local_wcs_cache/
'wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits exists and is non-empty
Saving wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits to local_wcs_cache/
'wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
The image scale is 5.79"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:18.438 +45:58:13.08
Second-epoch image center 00:00:19.655 +45:58:10.14
Angular distance between the image centers 0.00 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 00:00:18.438 +45:58:13.08
Second-epoch image center 00:00:18.710 +45:58:12.23
Angular distance between the image centers 0.00 deg.
###################################
Running solve_plate_with_UCAC5
Calibrating the magnitude scale
Found non-empty wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.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_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits and wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.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_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits and wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits.cat
Found non-empty wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits and wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits.cat
The reference image (wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits) and catalog (wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits.cat) found
'wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.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 68 out of 24062 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.782966
a=0.000000 b=1.000000 c=22.782966
From vast_summary.log: estimated ref. image limiting mag.: -10.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.26
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.26
____ 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 27 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits
2.1 pix And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits
2.5 pix fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
2.5 pix fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
All-image limiting magnitude estimate: 12.1 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_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
'wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
Preparing the HTML report for the field And-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out31610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31705.dat to exclusion_list_local.txt
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Considering the candidate 31610_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31610_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31610_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31610_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31610_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31645_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 31645_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 31647_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31647_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31647_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31647_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31647_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31651_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 31651_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 31652_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31652_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31652_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31652_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31652_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31657_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31657_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31657_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31657_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31657_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31658_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31658_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31658_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31658_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31658_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31661_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31661_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31661_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31661_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31661_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31665_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 31665_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 00:28:02.68 +44:23:11.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31666_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31666_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31666_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31666_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31666_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31667_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31667_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31667_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31667_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31667_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31671_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31671_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31671_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31671_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31671_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31674_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31674_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31674_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31674_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31674_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31677_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 31677_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 31678_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31678_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31678_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31678_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31678_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31679_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31679_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31679_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31679_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31679_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31680_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31680_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31680_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31680_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31680_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31682_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31682_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31682_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31682_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31682_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31689_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31689_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31689_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31689_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31689_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31692_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31692_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31692_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31692_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31692_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31694_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31694_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31694_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31694_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31694_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31696_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31696_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31696_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31696_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31696_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31697_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31697_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31697_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31697_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31697_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 31699_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 31699_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 31705_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 31705_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/31705_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/31705_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/31705_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
Prepared the HTML report for the field And-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:20:42.41 +50:30:39.8
00:08:05.75 +45:51:21.7
00:09:19.22 +46:24:05.3
23:25:21.53 +49:41:02.2
00:21:40.43 +46:18:43.3
00:22:01.68 +45:29:22.5
00:14:11.12 +45:24:09.7
00:06:41.67 +45:19:58.7
00:07:32.84 +47:41:55.2
23:39:19.92 +50:59:06.8
00:35:53.53 +48:58:06.5
00:29:48.42 +50:12:04.5
00:17:07.69 +48:33:13.7
00:02:46.58 +46:47:49.5
23:59:18.08 +45:47:25.5
00:06:50.69 +47:01:28.3
00:15:45.58 +46:23:39.1
00:11:32.13 +46:42:40.0
00:02:57.34 +47:55:08.5
23:16:13.85 +49:58:20.8
23:56:43.00 +45:32:21.8
23:47:04.45 +43:03:37.0
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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/2025-12-18/LIGHT/calibrated/platesolved/And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits
Creating symlink local_wcs_cache/wcs_And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits
Creating symlink local_wcs_cache/wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Creating symlink local_wcs_cache/wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits exists and is non-empty
wcs_And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits exists and is non-empty
The image scale is 5.79"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:18.438 +45:58:13.08
Second-epoch image center 00:00:19.655 +45:58:10.14
Angular distance between the image centers 0.00 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 00:00:18.438 +45:58:13.08
Second-epoch image center 00:00:18.710 +45:58:12.23
Angular distance between the image centers 0.00 deg.
###################################
Running solve_plate_with_UCAC5
Calibrating the magnitude scale
Found non-empty wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.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_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits and wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.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_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits and wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits.cat
Found non-empty wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits and wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits.cat
The reference image (wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits) and catalog (wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits.cat) found
'wcs_And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.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-2 143 out of 165931 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 20.844937
a=0.000000 b=1.000000 c=20.844937
From vast_summary.log: estimated ref. image limiting mag.: -7.81
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.03
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.03
____ 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 295 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits
1.9 pix And-01-Q1b1x1_2025-12-18_22-16-22_20.00sec_-14.90C_LIGHT_0099.fits
2.2 pix fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
2.2 pix fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
All-image limiting magnitude estimate: 12.7 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_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/wcs_fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
'wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2025-12-26_CI_And-01-Q1b1x1_195714_TTUQ1b1x1_9814_hEWuwgsr/wcs_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
Preparing the HTML report for the field And-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out190943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out176445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191403.dat to exclusion_list_local.txt
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190165_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190165_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190165_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190165_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190165_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190178_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190178_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190178_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190178_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190178_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190199_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190199_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190201_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190201_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190201_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190201_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190201_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190206_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190206_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 190207_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190207_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 190209_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190209_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 190210_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190210_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 190213_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190213_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 190214_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190214_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 190219_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190219_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190219_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190219_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190219_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190220_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190220_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190220_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190220_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190220_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190221_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190221_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190221_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190221_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190221_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190223_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190223_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 190225_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190225_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 190226_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190226_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 190228_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190228_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 190231_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190231_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190231_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190231_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190231_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190232_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190232_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190232_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190232_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190232_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190235_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190235_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 190242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190244_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190244_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190244_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190244_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190244_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190247_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190247_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 190252_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190252_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 190256_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190256_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 190263_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190263_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190263_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190263_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190263_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190266_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190266_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 190269_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190269_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190269_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190269_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190269_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190284_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190284_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (38.7") between the two second-epoch detections
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Considering the candidate 190291_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190291_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190291_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190291_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190291_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190292_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190292_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 190295_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190295_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 190299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190304_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190304_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190304_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190304_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190304_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190306_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190306_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 190308_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190308_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (35.3") between the two second-epoch detections
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Considering the candidate 190309_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190309_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190309_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190309_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190309_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190312_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190312_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (31.4") between the two second-epoch detections
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Considering the candidate 190321_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190321_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190321_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190321_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190321_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190327_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190327_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190327_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190327_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190327_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190329_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190329_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 190331_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190331_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190331_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190331_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190331_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190334_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190334_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190334_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190334_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190334_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190339_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190339_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 190341_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190341_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 190343_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190343_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 190345_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190345_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 190347_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190347_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 190351_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190351_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190351_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190351_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190351_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190356_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190356_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190356_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190356_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190356_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190357_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190357_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190357_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190357_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190357_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190358_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190358_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (40.9") between the two second-epoch detections
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Considering the candidate 190363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190364_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190364_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190364_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190364_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190364_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190369_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190369_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190369_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190369_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190369_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190370_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190370_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 190371_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190371_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 190372_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190372_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 190373_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190373_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 190376_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190376_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190376_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190376_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190376_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190379_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190379_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190379_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190379_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190379_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190380_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190380_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (35.8") between the two second-epoch detections
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Considering the candidate 190383_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190383_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190383_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190383_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190383_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190385_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190385_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (31.0") between the two second-epoch detections
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Considering the candidate 190392_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190392_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190392_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190392_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190392_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190395_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190395_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 190396_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190396_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190396_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190396_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190396_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190398_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190398_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190398_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190398_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190398_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190399_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190399_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190399_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190399_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190399_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190400_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190400_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 190406_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190406_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 190408_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190408_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 190409_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190409_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 190411_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190411_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190411_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190411_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190411_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190412_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190412_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190412_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190412_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190412_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190430_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190430_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 190436_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190436_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 190475_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190475_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (42.7") between the two second-epoch detections
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Considering the candidate 190476_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190476_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 190478_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190478_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
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Considering the candidate 190484_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190484_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190484_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190484_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190484_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190498_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190498_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190498_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190498_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190498_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190502_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190502_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190502_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190502_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190502_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190511_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190511_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190511_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190511_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190511_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190514_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190514_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 190515_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190515_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 190531_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190531_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (30.5") between the two second-epoch detections
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Considering the candidate 190535_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190535_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190535_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190535_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190535_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190544_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190544_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190544_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190544_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190544_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190547_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190547_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 190554_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190554_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 190561_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190561_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 190570_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190570_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (40.6") between the two second-epoch detections
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Considering the candidate 190576_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190576_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 190577_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190577_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190577_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190577_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190577_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190580_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190580_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190580_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190580_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190580_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190590_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190590_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 190592_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190592_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 190594_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190594_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 190605_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190605_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190605_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190605_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190605_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190610_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190610_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 190618_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190618_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190618_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190618_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190618_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190632_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190632_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 190638_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190638_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
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Considering the candidate 190651_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190651_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 190655_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190655_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 190659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190659_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190661_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190661_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 190665_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190665_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 190666_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190666_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 190671_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190671_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (51.3") between the two second-epoch detections
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Considering the candidate 190674_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190674_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 190681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190681_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190685_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190685_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190685_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190685_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190685_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190688_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190688_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 190691_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190691_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 190693_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190693_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 190695_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190695_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 190702_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190702_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190702_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190702_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190702_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190708_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190708_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (40.5") between the two second-epoch detections
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Considering the candidate 190713_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190713_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190713_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190713_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190713_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190717_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190717_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
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Considering the candidate 190720_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190720_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 190723_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190723_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 190729_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190729_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190729_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190729_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190729_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190742_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190742_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 190743_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190743_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190743_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190743_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190743_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190750_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190750_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 190753_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190753_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 190758_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190758_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190758_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190758_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190758_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190764_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190764_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (35.8") between the two second-epoch detections
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Considering the candidate 190769_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190769_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190769_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190769_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190769_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190770_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190770_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (31.3") between the two second-epoch detections
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Considering the candidate 190772_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190772_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190772_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190772_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190772_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190785_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190785_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 190787_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190787_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 190805_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190805_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 190808_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190808_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190808_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190808_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190808_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190812_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190812_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190812_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190812_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190812_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190816_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190816_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190816_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190816_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190816_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190817_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190817_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 190823_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190823_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 190826_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190826_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190826_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190826_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190826_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190830_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190830_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 190837_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190837_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 190838_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190838_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (36.9") between the two second-epoch detections
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Considering the candidate 190843_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190843_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190843_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190843_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190843_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190852_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190852_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 190858_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190858_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190858_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190858_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190858_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190862_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190862_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190862_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190862_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190862_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190864_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190864_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190864_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190864_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190864_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190865_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190865_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190865_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190865_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190865_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190869_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190869_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 190871_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190871_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190871_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190871_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190871_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190877_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190877_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190877_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190877_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190877_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190878_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190878_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190878_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190878_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190878_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190887_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190887_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 190889_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190889_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 190892_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190892_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (30.4") between the two second-epoch detections
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Considering the candidate 190894_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190894_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 190896_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190896_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 190898_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190898_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 190904_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190904_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190904_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190904_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190904_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190905_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190905_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190905_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190905_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190905_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190910_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190910_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190910_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190910_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190910_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190913_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190913_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 190916_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190916_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 190918_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190918_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190918_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190918_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190918_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190919_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190919_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (47.6") between the two second-epoch detections
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Considering the candidate 190924_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190924_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (31.0") between the two second-epoch detections
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Considering the candidate 190929_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190929_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190929_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190929_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190929_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190938_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190938_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 190943_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190943_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 190952_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190952_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 190955_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190955_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 190956_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190956_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 190959_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190959_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190959_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190959_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190959_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190963_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190963_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 190968_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190968_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 190988_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190988_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190988_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190988_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190988_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 190989_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190989_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 190991_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 190991_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 190994_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 190994_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/190994_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/190994_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/190994_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191001_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191001_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 191002_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191002_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191002_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191002_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191002_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191011_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191011_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 191013_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191013_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 191015_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191015_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (33.9") between the two second-epoch detections
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Considering the candidate 191018_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191018_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 191027_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191027_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191027_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191027_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191027_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191028_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191028_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191028_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191028_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191028_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191030_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191030_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 191036_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191036_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (52.9") between the two second-epoch detections
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Considering the candidate 191037_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191037_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191037_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191037_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191037_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191047_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191047_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191047_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191047_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191047_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191049_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191049_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191049_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191049_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191049_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191053_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191053_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 191058_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191058_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191058_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191058_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191058_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191062_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191062_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191062_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191062_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191062_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191066_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191066_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (31.3") between the two second-epoch detections
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Considering the candidate 191067_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191067_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191067_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191067_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191067_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191069_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191069_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 191076_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191076_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 191078_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191078_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (35.5") between the two second-epoch detections
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Considering the candidate 191082_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191082_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191082_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191082_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191082_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191084_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191084_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 191092_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191092_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191092_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191092_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191092_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191095_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191095_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 191096_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191096_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191096_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191096_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191096_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191099_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191099_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191099_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191099_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191099_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191100_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191100_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 191101_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191101_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 191102_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191102_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
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Considering the candidate 191111_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191111_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191111_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191111_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191111_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191114_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191114_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191114_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191114_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191114_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191115_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191115_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191115_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191115_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191115_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191118_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191118_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 191125_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191125_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 191128_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191128_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191128_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191128_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191128_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191130_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191130_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191130_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191130_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191130_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191131_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191131_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 191134_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191134_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191134_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191134_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191134_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191136_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191136_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 191150_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191150_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191150_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191150_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191150_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191153_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191153_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 191155_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191155_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 191156_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191156_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 191161_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191161_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 191163_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191163_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 191165_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191165_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 191166_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191166_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 191168_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191168_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (40.2") between the two second-epoch detections
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Considering the candidate 191170_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191170_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 191171_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191171_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 191175_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191175_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191175_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191175_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191175_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191176_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191176_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191176_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191176_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191176_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191178_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191178_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (39.3") between the two second-epoch detections
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Considering the candidate 191180_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191180_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 191182_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191182_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191182_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191182_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191182_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191184_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191184_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 191190_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191190_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191190_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191190_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191190_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191196_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191196_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 191199_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191199_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 191201_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191201_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 191209_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191209_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191209_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191209_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191209_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191214_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191214_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 191222_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191222_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191222_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191222_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191222_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191226_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191226_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 191228_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191228_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 191235_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191235_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 191236_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191236_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (39.9") between the two second-epoch detections
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Considering the candidate 191242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191242_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191250_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191250_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 191259_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191259_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191259_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191259_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191259_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191261_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191261_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (31.4") between the two second-epoch detections
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Considering the candidate 191270_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191270_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 191272_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191272_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 191278_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191278_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 191280_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191280_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 191287_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191287_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191287_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191287_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191287_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191290_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191290_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 191297_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191297_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (37.9") between the two second-epoch detections
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Considering the candidate 191298_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191298_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 191299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191299_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191304_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191304_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 191307_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191307_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 191313_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191313_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 191315_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191315_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 191318_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191318_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 191320_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191320_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 191322_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191322_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 191335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191335_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191337_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191337_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191337_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191337_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191337_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191345_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191345_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 191354_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191354_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 191356_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191356_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 191363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191363_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191369_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191369_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 191370_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191370_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191370_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191370_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191370_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191375_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191375_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191375_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191375_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191375_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191379_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191379_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 191380_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191380_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 191389_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191389_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191389_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191389_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191389_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191393_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191393_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191393_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191393_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191393_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191401_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191401_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 191403_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 191403_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
Successfully moved And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.png to transient_report/191403_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_reference.png
The output file transient_report/And-01-Q1b1x1_2025-12-18_22-15-52_20.00sec_-14.90C_LIGHT_0098.fits_preview.png already exist
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.png to transient_report/191403_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery1.png
Successfully moved fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.png to transient_report/191403_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051_discovery2.png
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Considering the candidate 191406_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191406_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 191407_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191407_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 191415_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191415_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 191416_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191416_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
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Considering the candidate 191424_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 191424_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 158954_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051
The candidate 158954_fd_And-01-Q1b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks