This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 11.24 22:22:13.85 +56:08:26.7
103.19602 -0.90428 galactic Cep Second-epoch detections are separated by 4.5" 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 J335.5671+56.1362 | 22:22:12.98 +56:08:13.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8III 1955ApJS....2...75M LF 4 +55 258
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!
Don'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 J335.5671+56.1362,2461093.5953,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J335.5671+56.1362 20260222.0953 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:22:13.85 +56:08:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 11.45 23:03:02.88 +54:07:26.4
107.37771 -5.44177 galactic Cas Second-epoch detections are separated by 2.1" 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 1996530498336877184 | 23:03:02.78 +54:07:07.2 (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 2026 02 22.0953* 23 03 02.88 +54 07 26.4 11.4 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
Gaia DR3 1996530498336877184,2461093.5953,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1996530498336877184 20260222.0953 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:03:02.88 +54:07:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J223030.83+550625.2,2461093.5953,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J223030.83+550625.2 20260222.0953 11.01CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:30:28.27 +55:06:20.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.85 21:46:54.39 +55:53:58.5
99.07833 1.82240 galactic Cep Second-epoch detections are separated by 3.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2175097955557202176 | 21:46:55.59 +55:53:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1928AnHar.100...49C HD 239768
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!
Don'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 2175097955557202176,2461093.5953,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2175097955557202176 20260222.0953 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:54.39 +55:53:58.5 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NSVS 3429299,2461093.5953,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3429299 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:00.25 +57:24:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 2174071836332109824,2461093.5953,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2174071836332109824 20260222.0953 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:28.59 +55:17:46.4 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.52 21:58:03.65 +52:33:28.2
98.25514 -1.80272 galactic Cyg Second-epoch detections are separated by 5.9" 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 J329.5244+52.5469 | 21:58:04.08 +52:33:14.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1927AnHar.100...33C HD 235678
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!
Don'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 J329.5244+52.5469,2461093.5953,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J329.5244+52.5469 20260222.0953 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:03.65 +52:33:28.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.56 22:04:39.21 +49:22:40.5
97.16521 -4.96565 galactic Lac Second-epoch detections are separated by 5.1" and 2.2 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 J331.1756+49.3857 | 22:04:38.97 +49:22:33.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1952CoRut..32....1H BD+48 3598
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!
Don'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 J331.1756+49.3857,2461093.5953,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J331.1756+49.3857 20260222.0953 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:39.21 +49:22:40.5 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.36 21:57:38.51 +52:49:17.2
98.36622 -1.55535 galactic Cyg Second-epoch detections are separated by 1.6" 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 J329.3941+52.8263 | 21:57:37.79 +52:49:14.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B0 1927AnHar.100...33C HD 235673
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!
Don'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 J329.3941+52.8263,2461093.5953,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J329.3941+52.8263 20260222.0953 10.36CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:38.51 +52:49:17.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 9.13 21:46:05.10 +49:56:01.9
95.14692 -2.66734 galactic Cyg Second-epoch detections are separated by 0.3" 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 | Gaia DR3 varaible 1980475635711688192 | 21:46:03.48 +49:55:49.3 (Gaia DR3) | LPV (Gaia DR3) | 2022yCat.1358....0G | Gaia3var=VARIABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: K5 1947AnDea...5....1L DO 40089
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!
Don'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 1980475635711688192,2461093.5953,9.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1980475635711688192 20260222.0953 9.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:05.10 +49:56:01.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
GU Cyg,2461093.5953,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GU Cyg 20260222.0953 9.56CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:06.19 +50:18:28.4 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 1979832245300519936,2461093.5953,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1979832245300519936 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:41.68 +50:24:12.4 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
BD+48 3592,2461093.5953,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BD+48 3592 20260222.0953 9.80CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:57.60 +49:24:14.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 9.88 21:46:46.19 +48:53:31.6
94.56053 -3.53614 galactic Cyg Second-epoch detections are separated by 0.7" 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 1978121546954871808 | 21:46:45.76 +48:53:23.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2 1952CoRut..32....1H BD+48 3503
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!
Don'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 1978121546954871808,2461093.5953,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1978121546954871808 20260222.0953 9.88CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:46.19 +48:53:31.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 2178601102686946688,2461093.5953,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2178601102686946688 20260222.0953 10.02CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:56.18 +58:30:08.8 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 1976375934808787072,2461093.5953,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1976375934808787072 20260222.0953 10.01CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:17.98 +48:51:32.5 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.10 21:52:36.05 +49:36:58.1
95.75757 -3.58154 galactic Cyg Second-epoch detections are separated by 2.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1979658458057827072 | 21:52:35.54 +49:36:54.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 1958PMcCO..13b....V AG+49 1882
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!
Don'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 1979658458057827072,2461093.5953,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1979658458057827072 20260222.0953 10.10CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:36.05 +49:36:58.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.10 21:45:46.41 +50:06:25.1
95.22040 -2.50277 galactic Cyg Second-epoch detections are separated by 1.1" 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 1980481270708866688 | 21:45:45.33 +50:06:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 1947AnDea...5....1L DO 40077
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!
Don'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 1980481270708866688,2461093.5953,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1980481270708866688 20260222.0953 10.10CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:46.41 +50:06:25.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J215517.16+493040.3,2461093.5953,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J215517.16+493040.3 20260222.0953 10.16CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:17.61 +49:30:37.7 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.17 21:59:51.57 +49:10:24.1
96.41469 -4.65917 galactic Cyg Second-epoch detections are separated by 0.4" 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 | ATO J329.9663+49.1805 | 21:59:51.14 +49:10:16.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J329.9663+49.1805,2461093.5953,10.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J329.9663+49.1805 20260222.0953 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:51.57 +49:10:24.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.22 21:53:46.36 +48:56:53.9
95.48795 -4.22198 galactic Cyg Second-epoch detections are separated by 1.0" and 2.2 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 J328.4232+48.9490 | 21:53:44.03 +48:56:54.1 (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!
Don'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 J328.4232+48.9490,2461093.5953,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J328.4232+48.9490 20260222.0953 10.22CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:46.36 +48:56:53.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
IRAS 22040+4839,2461093.5953,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IRAS 22040+4839 20260222.0953 10.30CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:00.84 +48:54:36.0 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.54 21:59:04.94 +55:10:00.2
99.96495 0.17374 galactic Cyg Second-epoch detections are separated by 1.2" 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 | ATO J329.7798+55.1713 | 21:59:06.85 +55:09:41.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8: 1928MeUpp..37....1S BD+54 2658
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!
Don'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 J329.7798+55.1713,2461093.5953,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J329.7798+55.1713 20260222.0953 10.54CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:04.94 +55:10:00.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 1976822508328378624,2461093.5953,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1976822508328378624 20260222.0953 10.38CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:34.29 +49:21:16.8 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.31 21:57:36.47 +49:37:49.6
96.40376 -4.07352 galactic Cyg Second-epoch detections are separated by 6.6" and 2.2 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 J329.4077+49.6193 | 21:57:36.63 +49:37:49.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 1952CoRut..32....1H BD+48 3558 J-Ks=0.197+/-0.025 (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!
Don'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 J329.4077+49.6193,2461093.5953,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J329.4077+49.6193 20260222.0953 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:36.47 +49:37:49.6 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.5953,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.0953 10.36CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:20.18 +49:12:33.5 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
BP Cyg,2461093.5953,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BP Cyg 20260222.0953 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:53.35 +48:57:36.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.46 21:48:44.92 +50:28:10.1
95.81808 -2.52940 galactic Cyg Second-epoch detections are separated by 1.7" 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 1980514152980002688 | 21:48:44.35 +50:28:07.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5: 1956PMcCO..13a....B AG+50 1697
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!
Don'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 1980514152980002688,2461093.5953,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1980514152980002688 20260222.0953 10.46CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:44.92 +50:28:10.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.52 21:52:01.59 +50:46:35.1
96.41546 -2.62073 galactic Cyg Second-epoch detections are separated by 0.3" and 2.2 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 J327.9921+50.7783 | 21:52:00.71 +50:46:42.2 (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!
Don'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 J327.9921+50.7783,2461093.5953,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J327.9921+50.7783 20260222.0953 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:01.59 +50:46:35.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.55 21:45:59.51 +50:54:39.0
95.76572 -1.91077 galactic Cyg Second-epoch detections are separated by 0.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.5186+50.9119 | 21:46:00.17 +50:54:39.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1927AnHar.100...33C HD 235608
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!
Don'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 J326.5186+50.9119,2461093.5953,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J326.5186+50.9119 20260222.0953 10.55CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:59.51 +50:54:39.0 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.64 22:07:09.77 +49:32:18.6
97.59073 -5.07690 galactic Lac Second-epoch detections are separated by 1.7" and 2.2 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 J331.7981+49.5247 | 22:07:08.95 +49:32:01.7 (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!
Don'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 J331.7981+49.5247,2461093.5953,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J331.7981+49.5247 20260222.0953 10.64CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:09.77 +49:32:18.6 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.87 22:12:56.77 +54:26:23.7
101.15338 -1.58862 galactic Lac Second-epoch detections are separated by 0.8" and 2.2 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 J333.2261+54.4347 | 22:12:57.43 +54:26:01.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0III 1955ApJS....2...75M LF 4 +54 155
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!
Don'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 J333.2261+54.4347,2461093.5953,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J333.2261+54.4347 20260222.0953 10.87CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:56.77 +54:26:23.7 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.71 21:49:03.57 +49:14:13.4
95.07044 -3.51121 galactic Cyg Second-epoch detections are separated by 0.6" 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 J327.2759+49.2444 | 21:49:04.35 +49:14:15.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1952CoRut..32....1H BD+48 3513
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!
Don'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 J327.2759+49.2444,2461093.5953,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J327.2759+49.2444 20260222.0953 10.71CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:03.57 +49:14:13.4 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.78 21:59:39.91 +49:06:18.0
96.34767 -4.69411 galactic Cyg Second-epoch detections are separated by 0.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.9142+49.1136 | 21:59:39.72 +49:06:12.1 (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!
Don'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 J329.9142+49.1136,2461093.5953,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J329.9142+49.1136 20260222.0953 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:39.91 +49:06:18.0 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
AM Lac,2461093.5953,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AM Lac 20260222.0953 11.01CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:39:02.50 +51:41:42.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.94 21:44:19.86 +58:33:23.7
100.53072 4.07571 galactic Cep Second-epoch detections are separated by 0.4" 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 | Gaia DR3 2178592925069564800 | 21:44:21.96 +58:33:05.6 (Gaia DR3) | E (local) | F (local) | Gaia3var=NOT_AVAILABLE SpType: F8 1932MeUpp..55....1S BD+57 2387
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!
Don'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 2178592925069564800,2461093.5953,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2178592925069564800 20260222.0953 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:19.86 +58:33:23.7 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NSV 25762,2461093.5953,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 25762 20260222.0953 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:18.20 +58:35:19.3 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.87 21:52:56.38 +49:03:11.7
95.44692 -4.05463 galactic Cyg Second-epoch detections are separated by 0.1" 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 | Gaia DR3 1979439895762036096 | 21:52:56.04 +49:03:05.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (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!
Don'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 1979439895762036096,2461093.5953,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1979439895762036096 20260222.0953 10.87CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:56.38 +49:03:11.7 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.92 22:07:26.15 +49:35:26.3
97.65743 -5.06064 galactic Lac Second-epoch detections are separated by 1.5" 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 1976746813828329216 | 22:07:24.75 +49:35:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 1976746813828329216,2461093.5953,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1976746813828329216 20260222.0953 10.92CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:26.15 +49:35:26.3 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.84 21:52:16.78 +48:53:47.1
95.26371 -4.10874 galactic Cyg Second-epoch detections are separated by 1.1" 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 1979367083167697536 | 21:52:18.92 +48:53:34.6 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B5 1952CoRut..32....1H BD+48 3529
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!
Don'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 1979367083167697536,2461093.5953,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1979367083167697536 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:16.78 +48:53:47.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
LT Cyg,2461093.5953,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LT Cyg 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:34.96 +49:55:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.89 21:55:45.52 +50:32:55.4
96.73642 -3.16744 galactic Cyg Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.9503+50.5549 | 21:55:44.97 +50:33:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J328.9503+50.5549,2461093.5953,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J328.9503+50.5549 20260222.0953 10.89CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:45.52 +50:32:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 11.04 21:48:15.66 +58:23:25.5
100.81694 3.61747 galactic Cep Second-epoch detections are separated by 0.3" 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 | ATO J327.0481+58.3915 | 21:48:16.74 +58:23:22.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0IV/V 1928MeUpp..37....1S BD+57 2401
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!
Don'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 J327.0481+58.3915,2461093.5953,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J327.0481+58.3915 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:15.66 +58:23:25.5 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J214900.08+484711.9,2461093.5953,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J214900.08+484711.9 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:00.73 +48:47:23.3 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J215609.07+485851.2,2461093.5953,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J215609.07+485851.2 20260222.0953 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:09.48 +48:58:59.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 1976493269011410304,2461093.5953,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1976493269011410304 20260222.0953 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:46.88 +49:15:28.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 11.04 21:47:50.40 +49:49:42.9
95.29619 -2.92962 galactic Cyg Second-epoch detections are separated by 2.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.9863+49.8247 | 21:47:54.32 +49:49:27.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K2 1958PMcCO..13b....V AG+49 1868
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!
Don'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 J326.9863+49.8247,2461093.5953,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J326.9863+49.8247 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:50.40 +49:49:42.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 11.05 21:48:03.87 +50:27:26.8
95.72649 -2.46917 galactic Cyg Second-epoch detections are separated by 0.3" 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 1980515355570622592 | 21:48:02.86 +50:27:18.2 (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!
Don'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 1980515355570622592,2461093.5953,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1980515355570622592 20260222.0953 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:03.87 +50:27:26.8 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J215940.37+493433.9,2461093.5953,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J215940.37+493433.9 20260222.0953 11.12CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:40.69 +49:34:41.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J220515.26+485508.7,2461093.5953,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J220515.26+485508.7 20260222.0953 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:15.87 +48:55:20.4 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J215347.34+503900.9,2461093.5953,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J215347.34+503900.9 20260222.0953 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:48.01 +50:39:05.5 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
Mis V1067,2461093.5953,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V1067 20260222.0953 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:38:07.72 +54:51:53.7 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J215300.54+510311.7,2461093.5953,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J215300.54+510311.7 20260222.0953 11.19CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:01.13 +51:03:17.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 11.15 21:46:51.04 +49:25:28.9
94.91369 -3.13674 galactic Cyg Second-epoch detections are separated by 0.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1978187826893138688 | 21:46:50.69 +49:25:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 1978187826893138688,2461093.5953,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1978187826893138688 20260222.0953 11.15CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:51.04 +49:25:28.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NSVS 5997944,2461093.5953,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5997944 20260222.0953 11.26CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:10.55 +49:13:40.4 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J220019.30+493352.7,2461093.5953,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J220019.30+493352.7 20260222.0953 11.26CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:19.68 +49:34:00.7 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J215631.94+495219.0,2461093.5953,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J215631.94+495219.0 20260222.0953 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:32.44 +49:52:27.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 1979853930603120896,2461093.5953,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1979853930603120896 20260222.0953 11.27CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:43.67 +50:40:20.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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 2026 02 22.0953* 23 14 50.74 +50 46 32.3 11.7 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
CL And,2461093.5953,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CL And 20260222.0953 11.65CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:50.74 +50:46:32.3 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J215349.71+485121.1,2461093.5953,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J215349.71+485121.1 20260222.0953 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:50.21 +48:51:30.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NSVS 3458825,2461093.5953,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3458825 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:40:59.58 +58:44:14.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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 2026 02 22.0953* 22 58 34.51 +54 00 33.2 11.0 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
ASASSN-V J225834.77+540034.8,2461093.5953,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J225834.77+540034.8 20260222.0953 11.02CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:58:34.51 +54:00:33.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J224113.54+504746.2,2461093.5953,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J224113.54+504746.2 20260222.0953 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:41:13.74 +50:47:55.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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 2026 02 22.0953* 23 14 47.50 +50 59 08.8 10.3 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
ASASSN-V J231448.90+505907.2,2461093.5953,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J231448.90+505907.2 20260222.0953 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:47.50 +50:59:08.8 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NT Lac,2461093.5953,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NT Lac 20260222.0953 10.79CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:29:54.02 +56:27:24.4 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
V0376 Lac,2461093.5953,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0376 Lac 20260222.0953 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:32:40.69 +55:12:35.0 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J224422.90+505125.3,2461093.5953,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J224422.90+505125.3 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:44:22.60 +50:51:28.5 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0953 2461093.5953 10.79 22:25:30.85 +53:30:14.2
102.18503 -3.38532 galactic Lac Second-epoch detections are separated by 0.9" and 2.2 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 | Large-amplitude variable Gaia DR2 2001798258552698752 | 22:25:32.47 +53:30:18.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: B8 1955ApJS....2...75M LF 4 +53 659
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!
Don'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 2001798258552698752,2461093.5953,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2001798258552698752 20260222.0953 10.79CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:25:30.85 +53:30:14.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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 2026 02 22.0953* 22 59 36.88 +51 40 20.2 11.3 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
CT And,2461093.5953,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CT And 20260222.0953 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:59:36.88 +51:40:20.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 1987961660625006976,2461093.5953,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1987961660625006976 20260222.0953 11.19CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:39:08.11 +49:35:42.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NSVS 3452061,2461093.5953,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3452061 20260222.0953 10.71CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:31:31.57 +53:41:45.3 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
LN Lac,2461093.5953,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LN Lac 20260222.0953 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:19:45.93 +54:42:16.8 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
LQ Lac,2461093.5953,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LQ Lac 20260222.0953 11.11CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:20:49.12 +52:50:53.0 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
AD Lac,2461093.5953,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AD Lac 20260222.0953 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:25:15.76 +52:08:43.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J224638.05+530435.3,2461093.5953,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J224638.05+530435.3 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:46:37.77 +53:04:37.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
AL Lac,2461093.5953,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AL Lac 20260222.0953 10.59CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:38:15.99 +52:13:39.0 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NSVS 3454648,2461093.5953,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3454648 20260222.0953 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:34:57.35 +55:55:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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 2026 02 22.0953* 23 07 24.16 +50 45 53.7 10.7 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
CX And,2461093.5953,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CX And 20260222.0953 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:07:24.16 +50:45:53.7 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J222230.13+551055.5,2461093.5953,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J222230.13+551055.5 20260222.0953 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:22:30.21 +55:10:55.3 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J221829.65+563232.4,2461093.5953,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J221829.65+563232.4 20260222.0953 10.36CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:18:29.89 +56:32:31.0 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J220602.29+584746.0,2461093.5953,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J220602.29+584746.0 20260222.0953 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:02.79 +58:47:44.5 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J224501.01+531416.5,2461093.5953,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J224501.01+531416.5 20260222.0953 11.22CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:45:00.77 +53:14:18.0 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
V0522 Cep,2461093.5953,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0522 Cep 20260222.0953 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:26:40.42 +58:31:30.8 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
YZ Lac,2461093.5953,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
YZ Lac 20260222.0953 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:11.39 +51:19:58.7 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J222310.76+542056.2,2461093.5953,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J222310.76+542056.2 20260222.0953 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:23:10.88 +54:20:56.5 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
V0434 Lac,2461093.5953,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0434 Lac 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:09.35 +54:37:16.0 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
FG Lac,2461093.5953,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FG Lac 20260222.0953 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:43:53.36 +52:58:18.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
AA Cep,2461093.5953,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AA Cep 20260222.0953 10.41CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:11.97 +56:30:46.8 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J223343.60+540052.7,2461093.5953,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J223343.60+540052.7 20260222.0953 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:33:43.46 +54:00:53.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
XY Lac,2461093.5953,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
XY Lac 20260222.0953 10.46CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:18:35.18 +52:48:14.8 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J223030.19+515927.1,2461093.5953,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J223030.19+515927.1 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:30:29.86 +51:59:28.4 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J223651.86+523705.0,2461093.5953,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J223651.86+523705.0 20260222.0953 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:36:51.65 +52:37:07.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J222223.30+553924.9,2461093.5953,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J222223.30+553924.9 20260222.0953 10.39CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:22:23.54 +55:39:23.7 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
AA Lac,2461093.5953,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AA Lac 20260222.0953 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:23:10.28 +52:41:37.3 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NSVS 3462609,2461093.5953,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3462609 20260222.0953 11.59CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:45:43.81 +58:56:57.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-12-12_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
Vend32,2461093.5953,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Vend32 20260222.0953 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:34:48.16 +53:00:26.3 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
WZ Lac,2461093.5953,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WZ Lac 20260222.0953 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:17.90 +54:11:53.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
LP Lac,2461093.5953,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LP Lac 20260222.0953 10.87CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:20:22.25 +54:15:10.8 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
DS Lac,2461093.5953,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DS Lac 20260222.0953 10.46CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:42:53.99 +55:18:41.3 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
GI Lac,2461093.5953,8.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GI Lac 20260222.0953 8.81CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:40:40.41 +50:00:42.6 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
II Lac,2461093.5953,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
II Lac 20260222.0953 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:17.56 +52:59:19.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 2005117301890342272,2461093.5953,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2005117301890342272 20260222.0953 11.44CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:24:13.68 +54:56:22.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
LX Lac,2461093.5953,9.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LX Lac 20260222.0953 9.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:59.18 +55:18:02.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NSVS 3470378,2461093.5953,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3470378 20260222.0953 11.38CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:54:56.25 +58:18:51.9 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J223930.30+531830.0,2461093.5953,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J223930.30+531830.0 20260222.0953 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:39:30.64 +53:18:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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 J221636.09+555449.4,2461093.5953,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J221636.09+555449.4 20260222.0953 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:36.41 +55:54:50.2 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
NSVS J2219532+554730,2461093.5953,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2219532+554730 20260222.0953 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:19:54.39 +55:47:24.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_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!
Don'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
OR Lac,2461093.5953,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OR Lac 20260222.0953 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:35:40.38 +55:29:24.1 ;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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png resample_wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20_00sec_-15_00C_LIGHT_0000_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.63312675 23.12.2025 03:11:32.151 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
First image: 2461032.63312675 23.12.2025 03:11:32.151 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
Last image: 2461093.59556737 22.02.2026 02:17:27.021 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 278
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.83
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 18 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 39643
Objects passed selection criteria: 39411
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 28966.8
Average stars matched: 28301.8 (97.7043 %)
Memory usage VmPeak: 141580 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Feb 21 20:21:56 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.63312675 23.12.2025 03:11:32.151 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
First image: 2461032.63312675 23.12.2025 03:11:32.151 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
Last image: 2461093.59556737 22.02.2026 02:17:27.021 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3340
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 327 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 284348
Objects passed selection criteria: 283386
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 198617
Average stars matched: 190599 (95.9631 %)
Memory usage VmPeak: 2027560 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Feb 21 20:39:11 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.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=
FRAME_EDGE_OFFSET_PIX= 100
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=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
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= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Lac-01-Q2b1x1
#######################################
########### Starting Lac-01-Q2b1x1 ###########
Processing Lac-01-Q2b1x1
server tau has sufficient free disk space available: 1150027 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1150027 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.png' -> 'transient_report/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits_preview.png'
Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
renamed 'Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.png' -> 'transient_report/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits_preview.png'
Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-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= 700.2830
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 933.2646
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1740.7928
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 796.5230
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1742.0862
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 795.7238
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.48584
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
No bad regions file found ../bad_region.lst
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
SExtractor catalog cache: saved Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat to cache
SExtractor catalog cache: saved Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.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: 2461093.59503536
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits exists and is non-empty
Saving wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits to local_wcs_cache/
'wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits' -> 'local_wcs_cache/wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits'
wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits exists and is non-empty
Saving wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits to local_wcs_cache/
'wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits' -> 'local_wcs_cache/wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits'
wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits exists and is non-empty
Saving wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits to local_wcs_cache/
'wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits' -> 'local_wcs_cache/wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits'
wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits exists and is non-empty
Saving wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits to local_wcs_cache/
'wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits' -> 'local_wcs_cache/wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:35:14.278 +53:59:17.30
Second-epoch image center 22:34:48.773 +54:00:15.44
Angular distance between the image centers 0.06 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 22:35:14.278 +53:59:17.30
Second-epoch image center 22:34:49.409 +54:00:03.68
Angular distance between the image centers 0.06 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:34:48.773 +54:00:15.44
Second-epoch second image center 22:34:49.409 +54:00:03.68
Angular distance between the image centers 0.00362 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits &> /tmp/tmp.EVQIZDWVcb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits &> /tmp/tmp.6qFXzaSB4K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits &> /tmp/tmp.C4qGU3bTAU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits &> /tmp/tmp.G3AB33ozHK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits and wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits and wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat
Found non-empty wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits and wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat
The reference image (wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits) and catalog (wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat) found
'wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.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 19459 out of 41811 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.963018
a=0.000000 b=1.000000 c=22.963018
From vast_summary.log: estimated ref. image limiting mag.: -7.83
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.13
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.13
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 247 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
2.1 pix Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
4.0 pix Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
4.0 pix Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
Limiting magnitude estimates:
15.1 mag. Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
15.1 mag. Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
14.0 mag. Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
13.9 mag. Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.EVQIZDWVcb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits' -> 'wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
WCS-calibrated image found: wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
Checking if the catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
WCS catalog name: wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=5547, passed=41811
Got 41811 stars (including 36213 good ones) from the SExtractor catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 41811 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits -region wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6qFXzaSB4K (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits' -> 'wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
WCS-calibrated image found: wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
Checking if the catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
WCS catalog name: wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=5546, passed=41703
Got 41703 stars (including 36121 good ones) from the SExtractor catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 41703 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 649 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.02"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 694 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.99"
Estimated accuracy of the plate solution: 2.15"
Excluding outliers - 632 stars left (next iteration limit 611)
The image catalog is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits -region wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.C4qGU3bTAU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
WCS-calibrated image found: wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
Checking if the catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
WCS catalog name: wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2032, passed=16714
Got 16714 stars (including 14671 good ones) from the SExtractor catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 16714 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.25"
Estimated accuracy of the plate solution: 1.38"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits -region wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.G3AB33ozHK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
Checking if the catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
WCS catalog name: wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2004, passed=16592
Got 16592 stars (including 14585 good ones) from the SExtractor catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 16592 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.22"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.21"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.21"
Estimated accuracy of the plate solution: 1.31"
Excluding outliers - 957 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits -region wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Lac-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out50068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52384.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out01367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52514.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 91s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 70s
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Considering the candidate 52203_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52203_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:05:10.13 +49:53:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 1.828 1976865492351234304 331.29291518244 +49.89496969701 10.1981 10.0637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52204_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52204_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52207_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52207_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:12:10.58 +48:59:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 5.539 1975919603122810624 333.04574179910 +48.99407872863 10.0602 9.6607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52208_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52208_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52210_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52210_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:00:17.29 +53:51:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 2.491 1981558379791926016 330.07135750901 +53.86593778440 9.9934 9.7266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52213_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52213_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:55:48.95 +56:32:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 4.911 2198916023117428480 328.95593406427 +56.53417884722 9.8832 9.5716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52214_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52214_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52215_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52215_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52216_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52216_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52217_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52217_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:06:21.89 +49:29:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.69, MAG_FAINT_SEARCH_LIMIT=11.67)GAIADR2_OUTPUT=# 4.305 1976651396831990016 331.59101111353 +49.49494993470 9.5544 9.3018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52218_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52218_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:53:07.97 +55:22:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 5.814 2174095956868778880 328.28571908976 +55.38015927024 9.6150 9.2174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52220_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52220_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52221_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52221_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:19:36.99 +58:54:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 1.408 2200374697087184896 334.90459539533 +58.90272129954 10.1260 9.8168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52224_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52224_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:35:33.91 +55:58:07.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)
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Considering the candidate 52225_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52225_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:05:48.20 +57:44:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 1.467 2199465435331350528 331.45144907061 +57.73564796276 9.8633 9.5826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52227_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52227_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:53:26.84 +51:30:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.52, MAG_FAINT_SEARCH_LIMIT=11.50)GAIADR2_OUTPUT=# 2.802 1980666675859193472 328.36297253126 +51.50295721844 9.0088 8.8835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52228_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52228_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:01:20.05 +56:49:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 5.387 2199026180441618688 330.33395016255 +56.82818702042 9.7054 9.4546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52229_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52229_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:00:51.93 +50:30:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.66, MAG_FAINT_SEARCH_LIMIT=11.64)GAIADR2_OUTPUT=# 4.980 1979978141056128000 330.21842495456 +50.51604658418 9.4442 9.1280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52230_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52230_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:04:02.61 +58:00:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.76, MAG_FAINT_SEARCH_LIMIT=11.74)GAIADR2_OUTPUT=# 1.421 2199521991455794048 331.01140813975 +58.00555747643 9.6540 9.4007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52231_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52231_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:02:29.89 +50:57:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 2.945 1980017345527536384 330.62557968541 +50.96489713486 9.5445 9.2353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52233_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52233_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 52234_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52234_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:55:21.00 +53:54:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 2.370 2173698723935698944 328.83674000045 +53.90287835966 9.4209 9.2427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52235_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52235_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 52236_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52236_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:46:11.57 +57:47:41.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)
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Considering the candidate 52237_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52237_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 52238_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52238_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52239_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52239_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:54.71 +54:34:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.56, MAG_FAINT_SEARCH_LIMIT=11.54)GAIADR2_OUTPUT=# 3.553 2173794037852280704 328.72844403459 +54.58227635883 9.3729 9.1827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52240_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52240_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 52241_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52241_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52243_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52243_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:05:38.64 +57:56:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)GAIADR2_OUTPUT=# 1.897 2199477426880145152 331.41193902216 +57.94410678691 9.4438 9.2442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52246_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52246_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:09:07.67 +58:01:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.48, MAG_FAINT_SEARCH_LIMIT=11.46)GAIADR2_OUTPUT=# 3.343 2199484848584377088 332.28214838705 +58.02227121105 9.6466 9.3009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52247_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52247_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:01:38.12 +50:10:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.42, MAG_FAINT_SEARCH_LIMIT=11.40)GAIADR2_OUTPUT=# 2.796 1979911002134040960 330.40919147918 +50.16795245995 9.2993 9.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52248_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52248_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:59:59.60 +50:31:53.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52250_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52250_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:47:06.23 +53:18:23.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52251_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52251_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:00:16.68 +55:35:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.51, MAG_FAINT_SEARCH_LIMIT=11.49)GAIADR2_OUTPUT=# 4.169 2198074106450867840 330.06763064967 +55.58408128919 9.3957 9.1787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52253_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52253_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:48:37.53 +51:36:23.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.35, MAG_FAINT_SEARCH_LIMIT=11.33)
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Considering the candidate 52254_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52254_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:15:03.55 +58:45:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.61, MAG_FAINT_SEARCH_LIMIT=11.59)GAIADR2_OUTPUT=# 1.600 2199625311192532480 333.76451976788 +58.75147701142 9.6641 9.3373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52255_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52255_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:56:49.16 +51:26:17.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52257_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52257_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 52259_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52259_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:56:22.25 +52:06:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.25, MAG_FAINT_SEARCH_LIMIT=11.23)GAIADR2_OUTPUT=# 2.212 1981127646113569408 329.09370886880 +52.11255626412 9.2536 8.9238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52260_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52260_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:03:57.23 +57:33:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.43, MAG_FAINT_SEARCH_LIMIT=11.41)GAIADR2_OUTPUT=# 4.657 2199088131051108992 330.99047997861 +57.55501738141 9.3181 9.0860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52261_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52261_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:53:57.57 +53:24:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.37, MAG_FAINT_SEARCH_LIMIT=11.35)GAIADR2_OUTPUT=# 4.632 2173593858016377216 328.48849220449 +53.41265076307 9.0439 8.7918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52262_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52262_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52263_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52263_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:49:04.26 +53:24:24.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52264_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52264_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:53:55.43 +54:17:57.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52265_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52265_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:02:47.93 +57:08:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.36, MAG_FAINT_SEARCH_LIMIT=11.34)GAIADR2_OUTPUT=# 4.682 2199060162223640448 330.70111529067 +57.13666919317 9.2945 9.0096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52266_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52266_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:51:23.54 +54:17:34.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)
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Considering the candidate 52267_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52267_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:49:58.83 +54:14:27.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52270_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52270_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:50:41.39 +54:56:36.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52272_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52272_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 52273_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52273_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 52275_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52275_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:55:06.59 +53:42:28.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52277_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52277_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:59:15.45 +50:50:05.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52278_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52278_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:56:48.03 +53:27:40.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52279_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52279_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:01:46.19 +57:39:49.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52280_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52280_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:42:54.12 +55:31:25.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52281_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52281_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 52282_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52282_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 52283_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52283_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:48:17.07 +54:23:18.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52284_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52284_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:56:45.38 +51:34:36.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52285_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52285_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:49:26.86 +54:22:56.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52287_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52287_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:52:30.64 +55:02:22.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52289_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52289_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:46:46.76 +49:18:30.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52290_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52290_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:38:55.37 +57:29:26.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52293_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52293_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:42:24.60 +57:44:09.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52294_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52294_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:49:03.87 +49:40:34.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52296_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52296_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:55:14.13 +50:29:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.45, MAG_FAINT_SEARCH_LIMIT=9.43)GAIADR2_OUTPUT=# 4.392 1979813626637908608 328.80735710704 +50.49714325209 7.1828 5.9533 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52297_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52297_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:59:33.28 +56:53:20.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52300_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52300_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:00:24.69 +49:03:11.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52301_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52301_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:56.65 +50:10:04.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52302_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52302_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:40:22.16 +57:34:54.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52304_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52304_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:50:22.83 +49:18:29.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52306_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52306_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:56:18.41 +58:24:47.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52307_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52307_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:50:36.03 +49:26:08.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52308_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52308_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:55:08.99 +50:18:45.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52309_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52309_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52310_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52310_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 52311_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52311_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:51:22.25 +49:53:01.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52314_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52314_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:56:34.81 +58:37:53.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52316_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52316_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52317_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52317_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:50:33.46 +51:00:00.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52320_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52320_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:49:59.15 +49:59:32.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52321_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52321_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52322_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52322_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:51:31.43 +49:40:36.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52323_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52323_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:51:20.92 +57:34:46.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52324_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52324_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:00:05.07 +48:54:09.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52325_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52325_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:56:31.06 +49:43:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.79, MAG_FAINT_SEARCH_LIMIT=10.77)GAIADR2_OUTPUT=# 1.348 1979555138325132032 329.12992112341 +49.72976061538 8.5807 7.7551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52328_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52328_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52330_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52330_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:39:27.47 +57:28:57.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52332_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52332_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:52:14.92 +49:48:17.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52333_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52333_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:47:58.22 +51:37:40.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52335_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52335_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52336_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52336_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52338_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52338_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52341_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52341_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:43:41.29 +58:14:24.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52342_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52342_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:57:29.22 +49:02:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.06, MAG_FAINT_SEARCH_LIMIT=11.04)GAIADR2_OUTPUT=# 0.930 1976474993937360256 329.37166572667 +49.04049758161 8.8927 8.1503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52344_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52344_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:42.43 +49:16:17.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52345_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52345_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52346_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52346_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52347_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52347_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52349_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52349_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52350_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52350_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52352_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52352_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:56:40.44 +49:40:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.23, MAG_FAINT_SEARCH_LIMIT=11.21)GAIADR2_OUTPUT=# 1.024 1979507859322952448 329.16885704451 +49.67980622768 9.0940 8.3823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52353_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52353_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52354_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52354_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:57:52.61 +50:33:41.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52356_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52356_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:52:44.15 +49:45:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)GAIADR2_OUTPUT=# 1.515 1979664264853835008 328.18460607431 +49.75451731474 9.0272 8.3305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52359_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52359_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:52:49.32 +49:52:08.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52360_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52360_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52361_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52361_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:43.20 +49:16:31.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52362_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52362_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52363_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52363_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52364_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52364_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52366_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52366_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:45:52.24 +51:27:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.35, MAG_FAINT_SEARCH_LIMIT=11.33)GAIADR2_OUTPUT=# 4.769 1980848026557961984 326.46637777749 +51.45022438762 9.0070 7.7379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52367_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52367_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52370_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52370_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:49:10.65 +48:47:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.31, MAG_FAINT_SEARCH_LIMIT=11.29)GAIADR2_OUTPUT=# 4.190 1977920061448426240 327.29463269357 +48.78490401403 8.7175 7.8932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52372_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52372_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:56.82 +49:59:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.40, MAG_FAINT_SEARCH_LIMIT=11.38)GAIADR2_OUTPUT=# 1.304 1979576097765177856 328.73729288334 +49.98823672490 9.2305 8.4373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52373_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52373_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:39:44.52 +58:14:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 1.021 2178573580536000384 324.93512878528 +58.24554431834 9.0343 8.7419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52374_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52374_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:53:30.12 +49:30:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.42, MAG_FAINT_SEARCH_LIMIT=11.40)GAIADR2_OUTPUT=# 2.784 1979466696352632960 328.37510332049 +49.50710408006 9.1134 8.2370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52376_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52376_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52378_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52378_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:59:15.45 +48:49:17.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.42, MAG_FAINT_SEARCH_LIMIT=11.40)
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Considering the candidate 52379_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52379_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52380_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52380_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:56:54.35 +50:14:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.32, MAG_FAINT_SEARCH_LIMIT=11.30)GAIADR2_OUTPUT=# 5.072 1979609495432146432 329.22861322770 +50.25007096861 9.0691 8.6450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52384_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52384_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:17.79 +49:34:43.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.47, MAG_FAINT_SEARCH_LIMIT=11.45)
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Considering the candidate 52385_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52385_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52388_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52388_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52389_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52389_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:59:16.00 +48:49:23.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)
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Considering the candidate 52391_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52391_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:49:46.02 +48:48:01.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52393_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52393_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:53:22.98 +49:20:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.61, MAG_FAINT_SEARCH_LIMIT=11.59)GAIADR2_OUTPUT=# 4.913 1979452574505887616 328.34752727739 +49.34686150141 9.3704 9.3023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52394_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52394_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:42:51.98 +57:01:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 4.367 2178217373124243328 325.71708001928 +57.01692852621 9.3411 9.1391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52396_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52396_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52398_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52398_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:47:30.00 +49:41:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 4.665 1979703641114778368 326.87598323968 +49.69156541182 9.1591 8.3850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52402_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52402_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52405_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52405_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:54.66 +49:30:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.76, MAG_FAINT_SEARCH_LIMIT=11.74)GAIADR2_OUTPUT=# 2.891 1979546754548336768 328.72738684461 +49.50378804579 9.5316 8.7702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52406_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52406_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:35.09 +48:49:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 3.696 1979377257956961280 328.64762341401 +48.81729244533 9.3733 9.0832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52407_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52407_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52408_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52408_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:45:52.01 +50:17:34.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52411_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52411_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52417_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52417_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52419_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52419_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:01:50.48 +49:10:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.83, MAG_FAINT_SEARCH_LIMIT=11.81)GAIADR2_OUTPUT=# 5.648 1976816598453293568 330.45929029892 +49.17936481288 9.7734 8.9286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52421_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52421_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 52424_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52424_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:55:30.73 +49:22:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 2.571 1979497207803504384 328.87851019290 +49.37146524938 9.4728 9.0111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52425_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52425_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52426_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52426_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52428_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52428_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:58:51.41 +49:25:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 4.696 1976507223366563712 329.71362782106 +49.41727915363 9.7029 8.8455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52429_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52429_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52430_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52430_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:53:25.90 +49:46:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 0.347 1979754665306688000 328.35802815151 +49.76696375942 9.7251 8.8950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52431_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52431_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52432_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52432_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52434_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52434_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52436_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52436_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:45:52.68 +50:17:41.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52438_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52438_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52439_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52439_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 52442_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52442_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52443_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52443_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52444_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52444_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:23:54.82 +57:00:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 1.583 2007780770036390016 335.97845424761 +57.00446695012 10.1267 8.5665 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52446_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52446_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:57:47.01 +49:08:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 2.950 1976477124241113216 329.44706568546 +49.14719957982 9.7668 9.3237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52449_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52449_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52450_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52450_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52451_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52451_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:56:50.85 +53:33:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 4.729 1990532795546563712 344.21390835517 +53.55334475360 10.4641 8.9227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52456_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52456_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:40:08.91 +58:00:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 1.369 2178550009755418880 325.03781358890 +58.01389237343 9.5349 9.2065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52457_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52457_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:02:32.96 +48:50:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 5.243 1976609684108389504 330.63656694576 +48.84760606171 9.9774 9.2839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52459_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52459_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52465_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52465_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:42:33.65 +58:14:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 1.707 2178536403298137216 325.63996662464 +58.24420983031 9.6147 9.2978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52472_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52472_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:55:44.49 +50:08:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 3.564 1979789609180738048 328.93690384044 +50.13774867886 9.9718 9.0523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52473_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52473_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52474_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52474_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:50:49.85 +49:17:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.08, MAG_FAINT_SEARCH_LIMIT=12.06)GAIADR2_OUTPUT=# 3.872 1979624957311892864 327.70934965720 +49.29070286870 9.5985 8.8269 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52475_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52475_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52476_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52476_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52477_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52477_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:49:08.94 +48:58:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 3.939 1979613927835196800 327.28886150190 +48.98013688395 9.3858 9.0209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52478_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52478_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52479_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52479_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52481_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52481_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:47:24.26 +48:58:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 5.023 1978127250671732224 326.85092305554 +48.97038649055 9.3844 8.6329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52484_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52484_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:59:49.91 +55:59:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 5.250 2008985353742088832 344.96040798748 +55.98916747771 10.7230 9.3029 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52486_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52486_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52488_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52488_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52491_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52491_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:15:01.38 +56:12:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.411 2006186272022639616 333.75481414903 +56.21061578411 10.3571 8.8864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52493_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52493_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:44.85 +50:49:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 2.064 1979868361703758720 328.68702637952 +50.82621248291 10.1799 8.9684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52494_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52494_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52495_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52495_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:47:45.78 +55:18:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 3.308 2003649561253998592 341.94235667697 +55.30360647715 12.3316 10.3560 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52499_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52499_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52500_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52500_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52505_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52505_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 23:02:12.45 +57:21:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 4.856 2010059233006106880 345.55433170463 +57.36216914981 10.7981 9.4155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52506_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52506_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52509_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52509_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:54:08.11 +49:36:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 4.339 1979561666674717824 328.53298000013 +49.61022104554 9.9540 9.0055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52511_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52511_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52513_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52513_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52514_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 52514_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 52517_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52517_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 21:55:18.57 +50:23:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 2.627 1979807991640864384 328.82748622020 +50.39894036943 10.2828 9.1172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52520_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52520_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:31:49.96 +56:59:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.67, MAG_FAINT_SEARCH_LIMIT=12.65)GAIADR2_OUTPUT=# 2.179 2007642953128321664 337.95875626675 +56.99695741423 10.8738 9.4779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52524_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52524_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:17:55.40 +52:39:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 2.746 2004286865685122688 334.48003696595 +52.65990962631 11.2318 9.7166 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52528_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52528_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 23:07:46.14 +51:14:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 5.509 1992080431180587776 346.94430805735 +51.24209080402 11.0682 9.6816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52534_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52534_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 23:04:55.65 +56:08:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 3.397 2009046376633378816 346.23356348769 +56.13587383149 11.2790 10.0520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52536_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52536_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 23:17:12.64 +53:41:12.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)
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Considering the candidate 52538_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 52538_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 23:16:48.61 +55:27:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 3.024 1997076371497531648 349.20397920419 +55.45021430066 11.9509 11.4874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 28693_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 28693_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:37:22.41 +51:32:48.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 16736_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 16736_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 32387_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 32387_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 27930_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 27930_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 08970_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 08970_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 13374_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 13374_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 31916_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 31916_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 20884_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 20884_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 26792_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 26792_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 38045_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 38045_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 19783_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 19783_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 15830_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 15830_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 23797_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 23797_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 26958_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 26958_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 21736_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 21736_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 25974_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 25974_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 10670_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 10670_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 30039_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 30039_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 13801_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 13801_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 08821_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 08821_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 01367_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 01367_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 50068_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 50068_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:23:42.43 +56:53:37.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)
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Considering the candidate 21150_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 21150_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 01860_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 01860_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 30734_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 30734_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 17332_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 17332_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 16222_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 16222_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 22329_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 22329_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 08869_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 08869_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 18386_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 18386_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 24008_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 24008_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 27532_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 27532_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 24263_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 24263_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 11909_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 11909_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 24420_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 24420_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 51372_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 51372_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 22699_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 22699_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 16257_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 16257_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 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 17979_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 17979_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 17739_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 17739_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 12596_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 12596_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 36472_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 36472_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 23151_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 23151_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 14768_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 14768_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 13195_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 13195_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 01792_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 01792_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 18426_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 18426_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:40:18.48 +53:50:45.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21165_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 21165_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 18104_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 18104_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:42:20.80 +53:54:32.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 11045_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 11045_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 25823_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
The candidate 25823_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001 did not pass the final checks
**** FOUND 22:23:34.12 +52:13:47.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 11438_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 11438_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
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Considering the candidate 12200_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
Preparing report for the candidate 12200_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001
make_report_in_HTML.sh Phase 2 (HTML assembly): 13s
make_report_in_HTML.sh TOTAL: 174s
Prepared the HTML report for the field Lac-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:06:02.79 +58:47:44.5
22:54:56.25 +58:18:51.9
22:26:40.42 +58:31:30.8
22:18:29.89 +56:32:31.0
22:08:11.97 +56:30:46.8
22:29:54.02 +56:27:24.4
22:34:57.35 +55:55:52.4
22:16:36.41 +55:54:50.2
22:19:54.39 +55:47:24.1
22:22:23.54 +55:39:23.7
22:35:40.38 +55:29:24.1
22:42:53.99 +55:18:41.3
22:21:59.18 +55:18:02.9
22:32:40.69 +55:12:35.0
22:22:30.21 +55:10:55.3
22:24:13.68 +54:56:22.1
22:19:45.93 +54:42:16.8
22:13:09.35 +54:37:16.0
22:58:34.51 +54:00:33.2
22:23:10.88 +54:20:56.5
22:20:22.25 +54:15:10.8
22:15:17.90 +54:11:53.1
22:33:43.46 +54:00:53.9
22:31:31.57 +53:41:45.3
22:25:30.85 +53:30:14.2
22:45:00.77 +53:14:18.0
22:39:30.64 +53:18:32.8
22:46:37.77 +53:04:37.4
22:43:53.36 +52:58:18.9
22:34:48.16 +53:00:26.3
22:06:17.56 +52:59:19.2
22:20:49.12 +52:50:53.0
22:18:35.18 +52:48:14.8
22:36:51.65 +52:37:07.9
22:23:10.28 +52:41:37.3
22:38:15.99 +52:13:39.0
22:59:36.88 +51:40:20.2
22:25:15.76 +52:08:43.1
22:30:29.86 +51:59:28.4
23:14:47.50 +50:59:08.8
23:07:24.16 +50:45:53.7
22:21:11.39 +51:19:58.7
22:44:22.60 +50:51:28.5
22:41:13.74 +50:47:55.2
22:40:40.41 +50:00:42.6
22:39:08.11 +49:35:42.2
22:45:43.81 +58:56:57.9
22:22:13.85 +56:08:26.7
23:03:02.88 +54:07:26.4
22:30:28.27 +55:06:20.2
21:46:54.39 +55:53:58.5
22:06:00.25 +57:24:17.1
21:52:28.59 +55:17:46.4
21:58:03.65 +52:33:28.2
22:04:39.21 +49:22:40.5
21:57:38.51 +52:49:17.2
21:46:05.10 +49:56:01.9
21:52:06.19 +50:18:28.4
21:52:41.68 +50:24:12.4
22:03:57.60 +49:24:14.1
21:46:46.19 +48:53:31.6
21:41:56.18 +58:30:08.8
21:55:17.98 +48:51:32.5
21:52:36.05 +49:36:58.1
21:45:46.41 +50:06:25.1
21:55:17.61 +49:30:37.7
21:59:51.57 +49:10:24.1
21:53:46.36 +48:56:53.9
22:06:00.84 +48:54:36.0
21:59:04.94 +55:10:00.2
22:01:34.29 +49:21:16.8
21:57:36.47 +49:37:49.6
21:54:20.18 +49:12:33.5
21:52:53.35 +48:57:36.9
21:48:44.92 +50:28:10.1
21:52:01.59 +50:46:35.1
21:45:59.51 +50:54:39.0
22:07:09.77 +49:32:18.6
22:12:56.77 +54:26:23.7
21:49:03.57 +49:14:13.4
21:59:39.91 +49:06:18.0
22:39:02.50 +51:41:42.2
21:44:19.86 +58:33:23.7
21:45:18.20 +58:35:19.3
21:52:56.38 +49:03:11.7
22:07:26.15 +49:35:26.3
21:52:16.78 +48:53:47.1
21:53:34.96 +49:55:18.8
21:55:45.52 +50:32:55.4
21:48:15.66 +58:23:25.5
21:49:00.73 +48:47:23.3
21:56:09.48 +48:58:59.1
22:00:46.88 +49:15:28.2
21:47:50.40 +49:49:42.9
21:48:03.87 +50:27:26.8
21:59:40.69 +49:34:41.2
22:05:15.87 +48:55:20.4
21:53:48.01 +50:39:05.5
22:38:07.72 +54:51:53.7
21:53:01.13 +51:03:17.9
21:46:51.04 +49:25:28.9
22:00:10.55 +49:13:40.4
22:00:19.68 +49:34:00.7
21:56:32.44 +49:52:27.2
21:53:43.67 +50:40:20.0
23:14:50.74 +50:46:32.3
21:53:50.21 +48:51:30.9
22:40:59.58 +58:44:14.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
SExtractor catalog cache: saved Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat to cache
SExtractor catalog cache: saved Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
Creating symlink local_wcs_cache/wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
Creating symlink local_wcs_cache/wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
Creating symlink local_wcs_cache/wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits exists and is non-empty
wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits exists and is non-empty
wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits exists and is non-empty
wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:35:14.278 +53:59:17.30
Second-epoch image center 22:34:48.773 +54:00:15.44
Angular distance between the image centers 0.06 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 22:35:14.278 +53:59:17.30
Second-epoch image center 22:34:49.409 +54:00:03.68
Angular distance between the image centers 0.06 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:34:48.773 +54:00:15.44
Second-epoch second image center 22:34:49.409 +54:00:03.68
Angular distance between the image centers 0.00362 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits &> /tmp/tmp.E64RkKUKt3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits &> /tmp/tmp.eqGEyh4R31
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits &> /tmp/tmp.lDxJNXB9sy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits &> /tmp/tmp.NV8aTjMeWC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits and wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.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_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits and wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat
Found non-empty wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits and wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat
The reference image (wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits) and catalog (wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat) found
'wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.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 20530 out of 306458 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.808268
a=0.000000 b=1.000000 c=22.808268
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3061 candidate transients before the final filtering. (Hard limit: 3000)
ERROR Too many candidates before filtering (3061)... Skipping SE run (default.sex.telephoto_lens_vSTL)
wait
############ /tmp/tmp.E64RkKUKt3 (5) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits' -> 'wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
WCS-calibrated image found: wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
Checking if the catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits
WCS catalog name: wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=64, blended=64996, passed=306394
Got 306394 stars (including 241013 good ones) from the SExtractor catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 306394 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits -region wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-11-32_20.00sec_-15.00C_LIGHT_0090.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eqGEyh4R31 (5) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits' -> 'wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
WCS-calibrated image found: wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
Checking if the catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits
WCS catalog name: wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=67, blended=65224, passed=308044
Got 308044 stars (including 242428 good ones) from the SExtractor catalog wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 308044 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 641 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.07"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 677 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.51"
Estimated accuracy of the plate solution: 1.69"
Excluding outliers - 615 stars left (next iteration limit 605)
The image catalog is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits -region wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lac-01-Q2b1x1_2025-12-22_21-12-12_20.00sec_-15.00C_LIGHT_0091.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.lDxJNXB9sy (5) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
WCS-calibrated image found: wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
Checking if the catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits
WCS catalog name: wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=20639, passed=94956
Got 94956 stars (including 74267 good ones) from the SExtractor catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 94956 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.23"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.22"
Estimated accuracy of the plate solution: 1.30"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits -region wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-16-41_20.00sec_-15.00C_LIGHT_0000.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NV8aTjMeWC (5) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
Checking if the catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits
WCS catalog name: wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=14, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=47, blended=20232, passed=94002
Got 94002 stars (including 73721 good ones) from the SExtractor catalog wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 94002 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.22"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.23"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.23"
Estimated accuracy of the plate solution: 1.30"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lac-01-Q2b1x1_201949_TTUQ2b1x1_10522_ABq434RV/Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits -region wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lac-01-Q2b1x1_2026-02-21_20-17-27_20.00sec_-15.00C_LIGHT_0001.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:06:02.79 +58:47:44.5
22:54:56.25 +58:18:51.9
22:26:40.42 +58:31:30.8
22:18:29.89 +56:32:31.0
22:08:11.97 +56:30:46.8
22:29:54.02 +56:27:24.4
22:34:57.35 +55:55:52.4
22:16:36.41 +55:54:50.2
22:19:54.39 +55:47:24.1
22:22:23.54 +55:39:23.7
22:35:40.38 +55:29:24.1
22:42:53.99 +55:18:41.3
22:21:59.18 +55:18:02.9
22:32:40.69 +55:12:35.0
22:22:30.21 +55:10:55.3
22:24:13.68 +54:56:22.1
22:19:45.93 +54:42:16.8
22:13:09.35 +54:37:16.0
22:58:34.51 +54:00:33.2
22:23:10.88 +54:20:56.5
22:20:22.25 +54:15:10.8
22:15:17.90 +54:11:53.1
22:33:43.46 +54:00:53.9
22:31:31.57 +53:41:45.3
22:25:30.85 +53:30:14.2
22:45:00.77 +53:14:18.0
22:39:30.64 +53:18:32.8
22:46:37.77 +53:04:37.4
22:43:53.36 +52:58:18.9
22:34:48.16 +53:00:26.3
22:06:17.56 +52:59:19.2
22:20:49.12 +52:50:53.0
22:18:35.18 +52:48:14.8
22:36:51.65 +52:37:07.9
22:23:10.28 +52:41:37.3
22:38:15.99 +52:13:39.0
22:59:36.88 +51:40:20.2
22:25:15.76 +52:08:43.1
22:30:29.86 +51:59:28.4
23:14:47.50 +50:59:08.8
23:07:24.16 +50:45:53.7
22:21:11.39 +51:19:58.7
22:44:22.60 +50:51:28.5
22:41:13.74 +50:47:55.2
22:40:40.41 +50:00:42.6
22:39:08.11 +49:35:42.2
22:45:43.81 +58:56:57.9
22:22:13.85 +56:08:26.7
23:03:02.88 +54:07:26.4
22:30:28.27 +55:06:20.2
21:46:54.39 +55:53:58.5
22:06:00.25 +57:24:17.1
21:52:28.59 +55:17:46.4
21:58:03.65 +52:33:28.2
22:04:39.21 +49:22:40.5
21:57:38.51 +52:49:17.2
21:46:05.10 +49:56:01.9
21:52:06.19 +50:18:28.4
21:52:41.68 +50:24:12.4
22:03:57.60 +49:24:14.1
21:46:46.19 +48:53:31.6
21:41:56.18 +58:30:08.8
21:55:17.98 +48:51:32.5
21:52:36.05 +49:36:58.1
21:45:46.41 +50:06:25.1
21:55:17.61 +49:30:37.7
21:59:51.57 +49:10:24.1
21:53:46.36 +48:56:53.9
22:06:00.84 +48:54:36.0
21:59:04.94 +55:10:00.2
22:01:34.29 +49:21:16.8
21:57:36.47 +49:37:49.6
21:54:20.18 +49:12:33.5
21:52:53.35 +48:57:36.9
21:48:44.92 +50:28:10.1
21:52:01.59 +50:46:35.1
21:45:59.51 +50:54:39.0
22:07:09.77 +49:32:18.6
22:12:56.77 +54:26:23.7
21:49:03.57 +49:14:13.4
21:59:39.91 +49:06:18.0
22:39:02.50 +51:41:42.2
21:44:19.86 +58:33:23.7
21:45:18.20 +58:35:19.3
21:52:56.38 +49:03:11.7
22:07:26.15 +49:35:26.3
21:52:16.78 +48:53:47.1
21:53:34.96 +49:55:18.8
21:55:45.52 +50:32:55.4
21:48:15.66 +58:23:25.5
21:49:00.73 +48:47:23.3
21:56:09.48 +48:58:59.1
22:00:46.88 +49:15:28.2
21:47:50.40 +49:49:42.9
21:48:03.87 +50:27:26.8
21:59:40.69 +49:34:41.2
22:05:15.87 +48:55:20.4
21:53:48.01 +50:39:05.5
22:38:07.72 +54:51:53.7
21:53:01.13 +51:03:17.9
21:46:51.04 +49:25:28.9
22:00:10.55 +49:13:40.4
22:00:19.68 +49:34:00.7
21:56:32.44 +49:52:27.2
21:53:43.67 +50:40:20.0
23:14:50.74 +50:46:32.3
21:53:50.21 +48:51:30.9
22:40:59.58 +58:44:14.2
########### Completed Lac-01-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
22:22:13.85 +56:08:26.7
23:03:02.88 +54:07:26.4
22:30:28.27 +55:06:20.2
21:46:54.39 +55:53:58.5
22:06:00.25 +57:24:17.1
21:52:28.59 +55:17:46.4
21:58:03.65 +52:33:28.2
22:04:39.21 +49:22:40.5
21:57:38.51 +52:49:17.2
21:46:05.10 +49:56:01.9
21:52:06.19 +50:18:28.4
21:52:41.68 +50:24:12.4
22:03:57.60 +49:24:14.1
21:46:46.19 +48:53:31.6
21:41:56.18 +58:30:08.8
21:55:17.98 +48:51:32.5
21:52:36.05 +49:36:58.1
21:45:46.41 +50:06:25.1
21:55:17.61 +49:30:37.7
21:59:51.57 +49:10:24.1
21:53:46.36 +48:56:53.9
22:06:00.84 +48:54:36.0
21:59:04.94 +55:10:00.2
22:01:34.29 +49:21:16.8
21:57:36.47 +49:37:49.6
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21:52:53.35 +48:57:36.9
21:48:44.92 +50:28:10.1
21:52:01.59 +50:46:35.1
21:45:59.51 +50:54:39.0
22:07:09.77 +49:32:18.6
22:12:56.77 +54:26:23.7
21:49:03.57 +49:14:13.4
21:59:39.91 +49:06:18.0
22:39:02.50 +51:41:42.2
21:44:19.86 +58:33:23.7
21:45:18.20 +58:35:19.3
21:52:56.38 +49:03:11.7
22:07:26.15 +49:35:26.3
21:52:16.78 +48:53:47.1
21:53:34.96 +49:55:18.8
21:55:45.52 +50:32:55.4
21:48:15.66 +58:23:25.5
21:49:00.73 +48:47:23.3
21:56:09.48 +48:58:59.1
22:00:46.88 +49:15:28.2
21:47:50.40 +49:49:42.9
21:48:03.87 +50:27:26.8
21:59:40.69 +49:34:41.2
22:05:15.87 +48:55:20.4
21:53:48.01 +50:39:05.5
22:38:07.72 +54:51:53.7
21:53:01.13 +51:03:17.9
21:46:51.04 +49:25:28.9
22:00:10.55 +49:13:40.4
22:00:19.68 +49:34:00.7
21:56:32.44 +49:52:27.2
21:53:43.67 +50:40:20.0
23:14:50.74 +50:46:32.3
21:53:50.21 +48:51:30.9
22:40:59.58 +58:44:14.2
22:58:34.51 +54:00:33.2
22:41:13.74 +50:47:55.2
23:14:47.50 +50:59:08.8
22:29:54.02 +56:27:24.4
22:32:40.69 +55:12:35.0
22:44:22.60 +50:51:28.5
22:25:30.85 +53:30:14.2
22:59:36.88 +51:40:20.2
22:39:08.11 +49:35:42.2
22:31:31.57 +53:41:45.3
22:19:45.93 +54:42:16.8
22:20:49.12 +52:50:53.0
22:25:15.76 +52:08:43.1
22:46:37.77 +53:04:37.4
22:38:15.99 +52:13:39.0
22:34:57.35 +55:55:52.4
23:07:24.16 +50:45:53.7
22:22:30.21 +55:10:55.3
22:18:29.89 +56:32:31.0
22:06:02.79 +58:47:44.5
22:45:00.77 +53:14:18.0
22:26:40.42 +58:31:30.8
22:21:11.39 +51:19:58.7
22:23:10.88 +54:20:56.5
22:13:09.35 +54:37:16.0
22:43:53.36 +52:58:18.9
22:08:11.97 +56:30:46.8
22:33:43.46 +54:00:53.9
22:18:35.18 +52:48:14.8
22:30:29.86 +51:59:28.4
22:36:51.65 +52:37:07.9
22:22:23.54 +55:39:23.7
22:23:10.28 +52:41:37.3
22:45:43.81 +58:56:57.9
22:34:48.16 +53:00:26.3
22:15:17.90 +54:11:53.1
22:20:22.25 +54:15:10.8
22:42:53.99 +55:18:41.3
22:40:40.41 +50:00:42.6
22:06:17.56 +52:59:19.2
22:24:13.68 +54:56:22.1
22:21:59.18 +55:18:02.9
22:54:56.25 +58:18:51.9
22:39:30.64 +53:18:32.8
22:16:36.41 +55:54:50.2
22:19:54.39 +55:47:24.1
22:35:40.38 +55:29:24.1
###################################################################################
22:22:13.85 +56:08:26.7 -- not an asteroid (will add it to exclusion list)
23:03:02.88 +54:07:26.4 -- not an asteroid (will add it to exclusion list)
22:30:28.27 +55:06:20.2 -- not an asteroid (will add it to exclusion list)
21:46:54.39 +55:53:58.5 -- not an asteroid (will add it to exclusion list)
22:06:00.25 +57:24:17.1 -- not an asteroid (will add it to exclusion list)
21:52:28.59 +55:17:46.4 -- not an asteroid (will add it to exclusion list)
21:58:03.65 +52:33:28.2 -- not an asteroid (will add it to exclusion list)
22:04:39.21 +49:22:40.5 -- not an asteroid (will add it to exclusion list)
21:57:38.51 +52:49:17.2 -- not an asteroid (will add it to exclusion list)
21:46:05.10 +49:56:01.9 -- not an asteroid (will add it to exclusion list)
21:52:06.19 +50:18:28.4 -- not an asteroid (will add it to exclusion list)
21:52:41.68 +50:24:12.4 -- not an asteroid (will add it to exclusion list)
22:03:57.60 +49:24:14.1 -- not an asteroid (will add it to exclusion list)
21:46:46.19 +48:53:31.6 -- not an asteroid (will add it to exclusion list)
21:41:56.18 +58:30:08.8 -- not an asteroid (will add it to exclusion list)
21:55:17.98 +48:51:32.5 -- not an asteroid (will add it to exclusion list)
21:52:36.05 +49:36:58.1 -- not an asteroid (will add it to exclusion list)
21:45:46.41 +50:06:25.1 -- not an asteroid (will add it to exclusion list)
21:55:17.61 +49:30:37.7 -- not an asteroid (will add it to exclusion list)
21:59:51.57 +49:10:24.1 -- not an asteroid (will add it to exclusion list)
21:53:46.36 +48:56:53.9 -- not an asteroid (will add it to exclusion list)
22:06:00.84 +48:54:36.0 -- not an asteroid (will add it to exclusion list)
21:59:04.94 +55:10:00.2 -- not an asteroid (will add it to exclusion list)
22:01:34.29 +49:21:16.8 -- not an asteroid (will add it to exclusion list)
21:57:36.47 +49:37:49.6 -- not an asteroid (will add it to exclusion list)
21:54:20.18 +49:12:33.5 -- not an asteroid (will add it to exclusion list)
21:52:53.35 +48:57:36.9 -- not an asteroid (will add it to exclusion list)
21:48:44.92 +50:28:10.1 -- not an asteroid (will add it to exclusion list)
21:52:01.59 +50:46:35.1 -- not an asteroid (will add it to exclusion list)
21:45:59.51 +50:54:39.0 -- not an asteroid (will add it to exclusion list)
22:07:09.77 +49:32:18.6 -- not an asteroid (will add it to exclusion list)
22:12:56.77 +54:26:23.7 -- not an asteroid (will add it to exclusion list)
21:49:03.57 +49:14:13.4 -- not an asteroid (will add it to exclusion list)
21:59:39.91 +49:06:18.0 -- not an asteroid (will add it to exclusion list)
22:39:02.50 +51:41:42.2 -- not an asteroid (will add it to exclusion list)
21:44:19.86 +58:33:23.7 -- not an asteroid (will add it to exclusion list)
21:45:18.20 +58:35:19.3 -- not an asteroid (will add it to exclusion list)
21:52:56.38 +49:03:11.7 -- not an asteroid (will add it to exclusion list)
22:07:26.15 +49:35:26.3 -- not an asteroid (will add it to exclusion list)
21:52:16.78 +48:53:47.1 -- not an asteroid (will add it to exclusion list)
21:53:34.96 +49:55:18.8 -- not an asteroid (will add it to exclusion list)
21:55:45.52 +50:32:55.4 -- not an asteroid (will add it to exclusion list)
21:48:15.66 +58:23:25.5 -- not an asteroid (will add it to exclusion list)
21:49:00.73 +48:47:23.3 -- not an asteroid (will add it to exclusion list)
21:56:09.48 +48:58:59.1 -- not an asteroid (will add it to exclusion list)
22:00:46.88 +49:15:28.2 -- not an asteroid (will add it to exclusion list)
21:47:50.40 +49:49:42.9 -- not an asteroid (will add it to exclusion list)
21:48:03.87 +50:27:26.8 -- not an asteroid (will add it to exclusion list)
21:59:40.69 +49:34:41.2 -- not an asteroid (will add it to exclusion list)
22:05:15.87 +48:55:20.4 -- not an asteroid (will add it to exclusion list)
21:53:48.01 +50:39:05.5 -- not an asteroid (will add it to exclusion list)
22:38:07.72 +54:51:53.7 -- not an asteroid (will add it to exclusion list)
21:53:01.13 +51:03:17.9 -- not an asteroid (will add it to exclusion list)
21:46:51.04 +49:25:28.9 -- not an asteroid (will add it to exclusion list)
22:00:10.55 +49:13:40.4 -- not an asteroid (will add it to exclusion list)
22:00:19.68 +49:34:00.7 -- not an asteroid (will add it to exclusion list)
21:56:32.44 +49:52:27.2 -- not an asteroid (will add it to exclusion list)
21:53:43.67 +50:40:20.0 -- not an asteroid (will add it to exclusion list)
23:14:50.74 +50:46:32.3 -- not an asteroid (will add it to exclusion list)
21:53:50.21 +48:51:30.9 -- not an asteroid (will add it to exclusion list)
22:40:59.58 +58:44:14.2 -- not an asteroid (will add it to exclusion list)
22:58:34.51 +54:00:33.2 -- not an asteroid (will add it to exclusion list)
22:41:13.74 +50:47:55.2 -- not an asteroid (will add it to exclusion list)
23:14:47.50 +50:59:08.8 -- not an asteroid (will add it to exclusion list)
22:29:54.02 +56:27:24.4 -- not an asteroid (will add it to exclusion list)
22:32:40.69 +55:12:35.0 -- not an asteroid (will add it to exclusion list)
22:44:22.60 +50:51:28.5 -- not an asteroid (will add it to exclusion list)
22:25:30.85 +53:30:14.2 -- not an asteroid (will add it to exclusion list)
22:59:36.88 +51:40:20.2 -- not an asteroid (will add it to exclusion list)
22:39:08.11 +49:35:42.2 -- not an asteroid (will add it to exclusion list)
22:31:31.57 +53:41:45.3 -- not an asteroid (will add it to exclusion list)
22:19:45.93 +54:42:16.8 -- not an asteroid (will add it to exclusion list)
22:20:49.12 +52:50:53.0 -- not an asteroid (will add it to exclusion list)
22:25:15.76 +52:08:43.1 -- not an asteroid (will add it to exclusion list)
22:46:37.77 +53:04:37.4 -- not an asteroid (will add it to exclusion list)
22:38:15.99 +52:13:39.0 -- not an asteroid (will add it to exclusion list)
22:34:57.35 +55:55:52.4 -- not an asteroid (will add it to exclusion list)
23:07:24.16 +50:45:53.7 -- not an asteroid (will add it to exclusion list)
22:22:30.21 +55:10:55.3 -- not an asteroid (will add it to exclusion list)
22:18:29.89 +56:32:31.0 -- not an asteroid (will add it to exclusion list)
22:06:02.79 +58:47:44.5 -- not an asteroid (will add it to exclusion list)
22:45:00.77 +53:14:18.0 -- not an asteroid (will add it to exclusion list)
22:26:40.42 +58:31:30.8 -- not an asteroid (will add it to exclusion list)
22:21:11.39 +51:19:58.7 -- not an asteroid (will add it to exclusion list)
22:23:10.88 +54:20:56.5 -- not an asteroid (will add it to exclusion list)
22:13:09.35 +54:37:16.0 -- not an asteroid (will add it to exclusion list)
22:43:53.36 +52:58:18.9 -- not an asteroid (will add it to exclusion list)
22:08:11.97 +56:30:46.8 -- not an asteroid (will add it to exclusion list)
22:33:43.46 +54:00:53.9 -- not an asteroid (will add it to exclusion list)
22:18:35.18 +52:48:14.8 -- not an asteroid (will add it to exclusion list)
22:30:29.86 +51:59:28.4 -- not an asteroid (will add it to exclusion list)
22:36:51.65 +52:37:07.9 -- not an asteroid (will add it to exclusion list)
22:22:23.54 +55:39:23.7 -- not an asteroid (will add it to exclusion list)
22:23:10.28 +52:41:37.3 -- not an asteroid (will add it to exclusion list)
22:45:43.81 +58:56:57.9 -- not an asteroid (will add it to exclusion list)
22:34:48.16 +53:00:26.3 -- not an asteroid (will add it to exclusion list)
22:15:17.90 +54:11:53.1 -- not an asteroid (will add it to exclusion list)
22:20:22.25 +54:15:10.8 -- not an asteroid (will add it to exclusion list)
22:42:53.99 +55:18:41.3 -- not an asteroid (will add it to exclusion list)
22:40:40.41 +50:00:42.6 -- not an asteroid (will add it to exclusion list)
22:06:17.56 +52:59:19.2 -- not an asteroid (will add it to exclusion list)
22:24:13.68 +54:56:22.1 -- not an asteroid (will add it to exclusion list)
22:21:59.18 +55:18:02.9 -- not an asteroid (will add it to exclusion list)
22:54:56.25 +58:18:51.9 -- not an asteroid (will add it to exclusion list)
22:39:30.64 +53:18:32.8 -- not an asteroid (will add it to exclusion list)
22:16:36.41 +55:54:50.2 -- not an asteroid (will add it to exclusion list)
22:19:54.39 +55:47:24.1 -- not an asteroid (will add it to exclusion list)
22:35:40.38 +55:29:24.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:41:56.18 +58:30:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:19.86 +58:33:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:18.20 +58:35:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:46.41 +50:06:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:59.51 +50:54:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:05.10 +49:56:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:46.19 +48:53:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:51.04 +49:25:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:54.39 +55:53:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:50.40 +49:49:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:03.87 +50:27:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:15.66 +58:23:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:44.92 +50:28:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:00.73 +48:47:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:03.57 +49:14:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:01.59 +50:46:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:06.19 +50:18:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:16.78 +48:53:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:28.59 +55:17:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:36.05 +49:36:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:41.68 +50:24:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:53.35 +48:57:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:56.38 +49:03:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:01.13 +51:03:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:34.96 +49:55:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:43.67 +50:40:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:46.36 +48:56:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:48.01 +50:39:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:50.21 +48:51:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:20.18 +49:12:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:17.61 +49:30:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:17.98 +48:51:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:45.52 +50:32:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:09.48 +48:58:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:32.44 +49:52:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:36.47 +49:37:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:38.51 +52:49:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:03.65 +52:33:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:04.94 +55:10:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:39.91 +49:06:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:40.69 +49:34:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:51.57 +49:10:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:10.55 +49:13:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:19.68 +49:34:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:46.88 +49:15:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:34.29 +49:21:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:57.60 +49:24:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:39.21 +49:22:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:15.87 +48:55:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:00.25 +57:24:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:00.84 +48:54:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:02.79 +58:47:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:17.56 +52:59:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:09.77 +49:32:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:26.15 +49:35:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:11.97 +56:30:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:56.77 +54:26:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:09.35 +54:37:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:17.90 +54:11:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:36.41 +55:54:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:29.89 +56:32:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:35.18 +52:48:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:45.93 +54:42:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:54.39 +55:47:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:22.25 +54:15:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:49.12 +52:50:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:11.39 +51:19:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:59.18 +55:18:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:13.85 +56:08:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:23.54 +55:39:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:30.21 +55:10:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:10.28 +52:41:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:10.88 +54:20:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:13.68 +54:56:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:15.76 +52:08:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:30.85 +53:30:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:40.42 +58:31:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:54.02 +56:27:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:30:28.27 +55:06:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:30:29.86 +51:59:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:31:31.57 +53:41:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:32:40.69 +55:12:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:33:43.46 +54:00:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:34:48.16 +53:00:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:34:57.35 +55:55:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:35:40.38 +55:29:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:36:51.65 +52:37:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:38:07.72 +54:51:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:38:15.99 +52:13:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:39:02.50 +51:41:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:39:08.11 +49:35:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:39:30.64 +53:18:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:40:40.41 +50:00:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:40:59.58 +58:44:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:41:13.74 +50:47:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:42:53.99 +55:18:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:43:53.36 +52:58:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:44:22.60 +50:51:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:45:00.77 +53:14:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:45:43.81 +58:56:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:46:37.77 +53:04:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:54:56.25 +58:18:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:58:34.51 +54:00:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:36.88 +51:40:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:02.88 +54:07:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:24.16 +50:45:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:47.50 +50:59:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:50.74 +50:46:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
21:41:56.18 +58:30:08.8 -- a known variable star
21:44:19.86 +58:33:23.7 -- not a known variable star
21:45:18.20 +58:35:19.3 -- a known variable star
21:45:46.41 +50:06:25.1 -- not a known variable star
21:45:59.51 +50:54:39.0 -- not a known variable star
21:46:05.10 +49:56:01.9 -- not a known variable star
21:46:46.19 +48:53:31.6 -- not a known variable star
21:46:51.04 +49:25:28.9 -- not a known variable star
21:46:54.39 +55:53:58.5 -- not a known variable star
21:47:50.40 +49:49:42.9 -- not a known variable star
21:48:03.87 +50:27:26.8 -- not a known variable star
21:48:15.66 +58:23:25.5 -- not a known variable star
21:48:44.92 +50:28:10.1 -- not a known variable star
21:49:00.73 +48:47:23.3 -- a known variable star
21:49:03.57 +49:14:13.4 -- not a known variable star
21:52:01.59 +50:46:35.1 -- not a known variable star
21:52:06.19 +50:18:28.4 -- a known variable star
21:52:16.78 +48:53:47.1 -- not a known variable star
21:52:28.59 +55:17:46.4 -- a known variable star
21:52:36.05 +49:36:58.1 -- not a known variable star
21:52:41.68 +50:24:12.4 -- a known variable star
21:52:53.35 +48:57:36.9 -- a known variable star
21:52:56.38 +49:03:11.7 -- not a known variable star
21:53:01.13 +51:03:17.9 -- a known variable star
21:53:34.96 +49:55:18.8 -- a known variable star
21:53:43.67 +50:40:20.0 -- a known variable star
21:53:46.36 +48:56:53.9 -- not a known variable star
21:53:48.01 +50:39:05.5 -- a known variable star
21:53:50.21 +48:51:30.9 -- a known variable star
21:54:20.18 +49:12:33.5 -- a known variable star
21:55:17.61 +49:30:37.7 -- a known variable star
21:55:17.98 +48:51:32.5 -- a known variable star
21:55:45.52 +50:32:55.4 -- not a known variable star
21:56:09.48 +48:58:59.1 -- a known variable star
21:56:32.44 +49:52:27.2 -- a known variable star
21:57:36.47 +49:37:49.6 -- not a known variable star
21:57:38.51 +52:49:17.2 -- not a known variable star
21:58:03.65 +52:33:28.2 -- not a known variable star
21:59:04.94 +55:10:00.2 -- not a known variable star
21:59:39.91 +49:06:18.0 -- not a known variable star
21:59:40.69 +49:34:41.2 -- a known variable star
21:59:51.57 +49:10:24.1 -- not a known variable star
22:00:10.55 +49:13:40.4 -- a known variable star
22:00:19.68 +49:34:00.7 -- a known variable star
22:00:46.88 +49:15:28.2 -- a known variable star
22:01:34.29 +49:21:16.8 -- a known variable star
22:03:57.60 +49:24:14.1 -- a known variable star
22:04:39.21 +49:22:40.5 -- not a known variable star
22:05:15.87 +48:55:20.4 -- a known variable star
22:06:00.25 +57:24:17.1 -- a known variable star
22:06:00.84 +48:54:36.0 -- a known variable star
22:06:02.79 +58:47:44.5 -- a known variable star
22:06:17.56 +52:59:19.2 -- a known variable star
22:07:09.77 +49:32:18.6 -- not a known variable star
22:07:26.15 +49:35:26.3 -- not a known variable star
22:08:11.97 +56:30:46.8 -- a known variable star
22:12:56.77 +54:26:23.7 -- not a known variable star
22:13:09.35 +54:37:16.0 -- a known variable star
22:15:17.90 +54:11:53.1 -- a known variable star
22:16:36.41 +55:54:50.2 -- a known variable star
22:18:29.89 +56:32:31.0 -- a known variable star
22:18:35.18 +52:48:14.8 -- a known variable star
22:19:45.93 +54:42:16.8 -- a known variable star
22:19:54.39 +55:47:24.1 -- a known variable star
22:20:22.25 +54:15:10.8 -- a known variable star
22:20:49.12 +52:50:53.0 -- a known variable star
22:21:11.39 +51:19:58.7 -- a known variable star
22:21:59.18 +55:18:02.9 -- a known variable star
22:22:13.85 +56:08:26.7 -- not a known variable star
22:22:23.54 +55:39:23.7 -- a known variable star
22:22:30.21 +55:10:55.3 -- a known variable star
22:23:10.28 +52:41:37.3 -- a known variable star
22:23:10.88 +54:20:56.5 -- a known variable star
22:24:13.68 +54:56:22.1 -- a known variable star
22:25:15.76 +52:08:43.1 -- a known variable star
22:25:30.85 +53:30:14.2 -- not a known variable star
22:26:40.42 +58:31:30.8 -- a known variable star
22:29:54.02 +56:27:24.4 -- a known variable star
22:30:28.27 +55:06:20.2 -- a known variable star
22:30:29.86 +51:59:28.4 -- a known variable star
22:31:31.57 +53:41:45.3 -- a known variable star
22:32:40.69 +55:12:35.0 -- a known variable star
22:33:43.46 +54:00:53.9 -- a known variable star
22:34:48.16 +53:00:26.3 -- a known variable star
22:34:57.35 +55:55:52.4 -- a known variable star
22:35:40.38 +55:29:24.1 -- a known variable star
22:36:51.65 +52:37:07.9 -- a known variable star
22:38:07.72 +54:51:53.7 -- a known variable star
22:38:15.99 +52:13:39.0 -- a known variable star
22:39:02.50 +51:41:42.2 -- a known variable star
22:39:08.11 +49:35:42.2 -- a known variable star
22:39:30.64 +53:18:32.8 -- a known variable star
22:40:40.41 +50:00:42.6 -- a known variable star
22:40:59.58 +58:44:14.2 -- a known variable star
22:41:13.74 +50:47:55.2 -- a known variable star
22:42:53.99 +55:18:41.3 -- a known variable star
22:43:53.36 +52:58:18.9 -- a known variable star
22:44:22.60 +50:51:28.5 -- a known variable star
22:45:00.77 +53:14:18.0 -- a known variable star
22:45:43.81 +58:56:57.9 -- a known variable star
22:46:37.77 +53:04:37.4 -- a known variable star
22:54:56.25 +58:18:51.9 -- a known variable star
22:58:34.51 +54:00:33.2 -- a known variable star
22:59:36.88 +51:40:20.2 -- a known variable star
23:03:02.88 +54:07:26.4 -- not a known variable star
23:07:24.16 +50:45:53.7 -- a known variable star
23:14:47.50 +50:59:08.8 -- a known variable star
23:14:50.74 +50:46:32.3 -- a known variable star
Found 31 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
108 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
No ../exclusion_list_TTUQ2.txt so we are not updating exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= YES
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.59503536 -observatory 500
23:23:17.15 -02:01:01.6 Mercury (-0.1mag)
23:04:07.62 -07:31:57.9 Venus (-3.9mag)
21:42:35.27 -14:53:58.0 Mars (1.1mag)
07:06:07.05 +22:54:18.1 Jupiter (-2.5mag)
00:05:24.33 -01:44:40.4 Saturn (1.0mag)
03:39:59.21 +19:21:42.7 Uranus (5.7mag)
00:03:40.34 -01:01:41.0 Neptune (7.8mag)
20:29:06.51 -22:59:35.4 Pluto (14.5mag)
01:50:21.85 +15:50:36.2 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 362 Feb 21 20:21 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.59503536:
07:06:09.38 +22:54:16.3 Io (5.4mag)
07:06:17.67 +22:53:59.0 Europa (5.5mag)
07:05:56.64 +22:54:45.7 Ganymede (4.9mag)
07:06:25.24 +22:53:54.3 Callisto (6.2mag)
07:09:15.72 +23:10:42.9 Himalia (15.0mag)
07:06:05.84 +22:54:22.7 Thebe (15.9mag)
07:08:40.85 +23:19:09.1 Elara (17.0mag)
07:01:40.40 +24:02:18.5 Pasiphae (17.0mag)
07:15:07.96 +22:42:16.9 Carme (18.1mag)
00:05:35.97 -01:44:45.1 Titan (8.8mag)
00:05:29.65 -01:44:39.1 Rhea (10.1mag)
00:05:19.57 -01:46:01.6 Iapetus (11.5mag)
00:05:24.94 -01:44:43.2 Hyperion (14.8mag)
00:07:28.63 -01:31:40.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 21 20:22 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.59503536:
08:45:19.26 +24:30:39.1 JWST
10:01:18.63 +35:21:45.9 Chandra
14:38:57.12 -62:35:47.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 21 20:21 spacecraft.txt
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Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461093.59503536 at 500
16:59:34.72 -11:03:46.4 17.5mag 10P/Tempel 2
03:37:15.31 +28:57:37.0 18.0mag 123P/West-Hartley
08:23:44.38 +60:43:58.9 18.4mag 124P/Mrkos
21:19:22.79 -07:39:46.6 22.1mag 141P/Machholz
01:21:01.04 +11:53:50.5 17.6mag 145P/Shoemaker-Levy 5
11:03:02.42 +30:34:08.2 17.9mag 164P/Christensen
09:33:09.95 -33:51:57.4 18.0mag 195P/Hill
15:52:03.60 -06:36:13.5 19.2mag 210P/Christensen
18:16:34.86 -21:28:43.1 17.3mag 218P/LINEAR
16:21:28.09 -18:11:01.4 15.2mag 235P/LINEAR
03:56:18.26 +27:43:51.6 17.8mag 240P/NEAT
15:17:33.58 +06:38:41.1 14.8mag 24P/Schaumasse
11:23:32.52 -03:23:15.1 17.4mag 29P/Schwassmann-Wachmann 1
07:03:48.31 +27:24:48.7 19.6mag 407P/PanSTARRS-Fuls
17:07:02.84 -11:19:15.9 17.6mag 40P/Vaisala 1
11:02:15.17 -08:52:04.9 16.6mag 43P/Wolf-Harrington
13:25:29.52 -05:49:27.8 20.0mag 489P/Denning
04:34:19.45 +48:34:51.3 17.8mag 493P/2024 Q2 (LONEOS)
06:04:21.78 +47:32:07.1 17.7mag 63P/Wild 1
23:14:29.46 -02:08:09.9 16.2mag 78P/Gehrels 2
20:01:17.01 -22:18:49.0 15.0mag 88P/Howell
15:27:52.90 -29:00:24.0 18.7mag P/2023 S1 (PanSTARRS)
04:43:26.77 -72:36:06.5 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:50.50 +31:12:53.6 18.2mag C/2017 K2 (PanSTARRS)
20:06:36.30 -65:11:31.6 18.1mag C/2020 V2 (ZTF)
17:21:38.93 +04:21:00.9 16.3mag C/2021 G2 (ATLAS)
03:35:38.20 +24:36:38.0 15.8mag C/2022 N2 (PanSTARRS)
09:08:14.46 +29:49:17.5 15.3mag C/2022 QE78 (ATLAS)
08:35:41.62 -06:34:12.8 16.7mag C/2022 R6 (PanSTARRS)
23:52:57.77 +48:26:36.9 18.0mag C/2023 C2 (ATLAS)
09:51:11.68 -20:46:29.6 17.5mag C/2023 F3 (ATLAS)
20:34:38.31 +61:14:30.7 17.3mag C/2023 H5 (Lemmon)
19:34:29.72 -03:24:14.2 16.1mag C/2023 R1 (PANSTARRS)
02:48:54.11 +35:40:35.9 18.5mag C/2023 RS61 (PanSTARRS)
21:01:21.24 +81:19:52.1 18.0mag C/2023 X2 (Lemmon)
06:39:14.81 +63:49:08.5 17.3mag C/2024 A1 (ATLAS)
01:56:19.80 -24:42:34.8 11.2mag C/2024 E1 (Wierzchos)
11:45:01.42 -02:35:30.2 18.1mag C/2024 G2 (ATLAS)
19:28:15.68 +00:39:05.6 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.83 -01:43:19.8 17.7mag C/2024 G6 (ATLAS)
19:53:25.21 +03:14:28.9 15.6mag C/2024 J3 (ATLAS)
02:47:12.77 -31:35:07.9 15.4mag C/2024 T5 (ATLAS)
16:25:15.42 -58:12:28.9 15.6mag C/2025 A6 (Lemmon)
04:50:30.17 +62:15:52.3 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
15:56:45.81 -13:04:07.1 14.8mag C/2025 L1 (ATLAS)
02:20:11.15 -19:05:29.2 16.7mag C/2025 Q3 (ATLAS)
02:09:30.13 +17:16:24.5 21.2mag C/2025 R2 (SWAN)
22:20:44.63 +17:39:09.7 16.4mag C/2025 R3 (PANSTARRS)
21:45:57.61 -16:49:41.5 21.5mag C/2025 T1 (ATLAS)
03:06:22.27 -20:35:41.3 18.3mag C/2026 A1 (MAPS)
21:02:49.15 +20:54:05.0 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 21 20:22 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
-rw-r--r-- 1 apache apache 6.2K Feb 21 20:21 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 21 20:21 tocp_transients_list.txt
