This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh
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 22.1488 2461093.6488 11.12 20:26:21.56 +66:28:43.2
100.59723 15.97145 galactic Cep Second-epoch detections are separated by 1.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246592668352465920 | 20:26:20.48 +66:28:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1956PMcCO..13a....B AG+66 958
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 2246592668352465920,2461093.6488,11.12,0.05,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
Gaia DR3 2246592668352465920 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:26:21.56 +66:28:43.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.93 20:39:55.26 +73:32:07.8
107.47712 18.80194 galactic Cep Second-epoch detections are separated by 5.3" and 3.4 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 2276182686622836480 | 20:39:56.59 +73:32:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1948UppAn...2d....S BD+73 913
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 2276182686622836480,2461093.6488,10.93,0.05,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 2276182686622836480 20260222.1488 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:39:55.26 +73:32:07.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.52 20:30:15.79 +66:44:12.1
101.03975 15.78293 galactic Cep Second-epoch detections are separated by 2.0" and 5.3 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 2246435128952498432 | 20:30:14.97 +66:44:07.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1956PMcCO..13a....B AG+66 961
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 2246435128952498432,2461093.6488,10.52,0.05,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
Gaia DR3 2246435128952498432 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:30:15.79 +66:44:12.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
IN Cep,2461093.6488,9.87,0.05,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
IN Cep 20260222.1488 9.87CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:29:33.52 +67:02:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
BS Dra,2461093.6488,10.37,0.05,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
BS Dra 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:56:26.86 +73:36:58.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.41 20:01:16.49 +72:54:15.9
105.45942 20.93701 galactic Dra Second-epoch detections are separated by 2.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2287868437938162048 | 20:01:18.24 +72:54:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1948UppAn...2d....S BD+72 928
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 2287868437938162048,2461093.6488,10.41,0.05,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
Gaia DR3 2287868437938162048 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:01:16.49 +72:54:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.32 20:22:25.21 +70:03:41.4
103.60634 18.13809 galactic Dra Second-epoch detections are separated by 3.3" and 4.4 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 2250586644340119936 | 20:22:27.38 +70:03:44.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1948UppAn...2d....S BD+69 1101
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 2250586644340119936,2461093.6488,10.32,0.05,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 2250586644340119936 20260222.1488 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:22:25.21 +70:03:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.39 20:27:22.59 +72:44:39.6
106.25888 19.15625 galactic Dra Second-epoch detections are separated by 4.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2276026422829346304 | 20:27:24.67 +72:44:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1925sdsl.book.....L BD+72 955
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 2276026422829346304,2461093.6488,10.39,0.05,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
Gaia DR3 2276026422829346304 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:22.59 +72:44:39.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.29 20:36:46.02 +65:25:39.3
100.29003 14.50845 galactic Cep Second-epoch detections are separated by 3.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2245492332091730048 | 20:36:44.74 +65:25:31.8 (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 2245492332091730048,2461093.6488,10.29,0.05,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 2245492332091730048 20260222.1488 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:36:46.02 +65:25:39.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.35 20:14:32.22 +70:50:20.6
103.98160 19.09351 galactic Dra Second-epoch detections are separated by 2.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251420967507259008 | 20:14:35.21 +70:50:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1926BHarO.834....4L BD+70 1112
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 2251420967507259008,2461093.6488,10.35,0.05,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 2251420967507259008 20260222.1488 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:14:32.22 +70:50:20.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.57 20:25:04.46 +72:56:16.7
106.34522 19.40055 galactic Dra Second-epoch detections are separated by 1.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2276082154324264576 | 20:25:07.12 +72:56:15.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3V 1925sdsl.book.....L BD+72 951
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 2276082154324264576,2461093.6488,10.57,0.05,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
Gaia DR3 2276082154324264576 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:04.46 +72:56:16.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.54 20:25:26.70 +73:13:53.6
106.62915 19.52404 galactic Dra Second-epoch detections are separated by 4.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2276105622025688832 | 20:25:29.19 +73:13:53.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1925sdsl.book.....L BD+72 952
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 2276105622025688832,2461093.6488,10.54,0.05,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
Gaia DR3 2276105622025688832 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:26.70 +73:13:53.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.59 20:30:34.81 +65:27:11.2
99.94148 15.05649 galactic Cep Second-epoch detections are separated by 3.0" and 5.1 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 2246206567973292160 | 20:30:33.18 +65:27:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3 1947AnDea...5....1L DO 38541
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 2246206567973292160,2461093.6488,10.59,0.05,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
Gaia DR3 2246206567973292160 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:30:34.81 +65:27:11.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.79 20:13:51.87 +72:28:28.7
105.48788 19.90710 galactic Dra Second-epoch detections are separated by 2.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275867367304256384 | 20:13:54.37 +72:28:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5V 1948UppAn...2d....S BD+72 944
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 2275867367304256384,2461093.6488,10.79,0.05,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
Gaia DR3 2275867367304256384 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:51.87 +72:28:28.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.79 20:25:40.31 +64:47:48.0
99.08047 15.13537 galactic Dra Second-epoch detections are separated by 0.7" and 5.3 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 2244664262398110464 | 20:25:41.36 +64:47:51.8 (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 2244664262398110464,2461093.6488,10.79,0.05,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
Gaia DR3 2244664262398110464 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:40.31 +64:47:48.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.85 20:03:01.33 +72:37:10.6
105.24126 20.69975 galactic Dra Second-epoch detections are separated by 5.1" and 4.5 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 2275828751254355328 | 20:03:02.72 +72:37:11.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1948UppAn...2d....S BD+72 931
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 2275828751254355328,2461093.6488,10.85,0.05,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 2275828751254355328 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:01.33 +72:37:10.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.79 20:20:36.24 +66:09:01.0
99.99146 16.29281 galactic Dra Second-epoch detections are separated by 0.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246479556093764352 | 20:20:39.30 +66:09:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+65 1019
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 2246479556093764352,2461093.6488,10.79,0.05,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
Gaia DR3 2246479556093764352 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:20:36.24 +66:09:01.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.17 19:54:15.53 +73:23:22.0
105.71604 21.59775 galactic Dra Second-epoch detections are separated by 5.1" and 4.5 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 2287952241339914624 | 19:54:17.09 +73:23:19.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5V 1948UppAn...2d....S BD+73 887
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 2287952241339914624,2461093.6488,11.17,0.05,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
Gaia DR3 2287952241339914624 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:15.53 +73:23:22.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J203659.19+651518.8,2461093.6488,11.02,0.05,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 J203659.19+651518.8 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:37:00.01 +65:15:24.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2250353681019455872,2461093.6488,11.13,0.05,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 2250353681019455872 20260222.1488 11.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:50.97 +69:35:48.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.26 20:20:57.02 +73:41:09.9
106.88280 20.02598 galactic Dra Second-epoch detections are separated by 4.9" and 4.4 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 2276317587251480832 | 20:20:59.50 +73:41:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5III 1948UppAn...2d....S [S48] 140
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 2276317587251480832,2461093.6488,11.26,0.05,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
Gaia DR3 2276317587251480832 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:20:57.02 +73:41:09.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2300118+700223,2461093.6488,11.71,0.05,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 J2300118+700223 20260222.1488 11.71CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:00:10.28 +70:02:27.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.46 20:03:44.77 +71:36:25.5
104.29030 20.21554 galactic Dra Second-epoch detections are separated by 3.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2251716426895634560 | 20:03:46.32 +71:36:24.4 (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: B:k 1948UppAn...2d....S BD+71 994
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 2251716426895634560,2461093.6488,11.46,0.05,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
Large-amplitude variable Gaia DR2 2251716426895634560 20260222.1488 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:44.77 +71:36:25.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2036382+681740,2461093.6488,11.50,0.05,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 J2036382+681740 20260222.1488 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:36:38.77 +68:17:39.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.52 20:04:23.02 +71:45:46.6
104.46313 20.23794 galactic Dra Second-epoch detections are separated by 2.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251719450555617152 | 20:04:24.35 +71:45:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1948UppAn...2d....S BD+71 995
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 2251719450555617152,2461093.6488,11.52,0.05,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
Gaia DR3 2251719450555617152 20260222.1488 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:04:23.02 +71:45:46.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2049408+721550,2461093.6488,11.62,0.05,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
NSVS J2049408+721550 20260222.1488 11.62CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:49:42.41 +72:15:49.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.50 21:51:16.86 +71:04:29.5
109.30098 13.14209 galactic Cep Second-epoch detections are separated by 2.3" and 4.3 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 2224563952889561600 | 21:51:17.28 +71:04:31.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2224563952889561600,2461093.6488,11.50,0.05,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 2224563952889561600 20260222.1488 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:16.86 +71:04:29.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V1232 Cep,2461093.6488,11.36,0.05,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
V1232 Cep 20260222.1488 11.36CV 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/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:32:58.85 +66:54:43.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-28-46_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2135423+683909,2461093.6488,11.57,0.05,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 J2135423+683909 20260222.1488 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:42.56 +68:39:08.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0555 Cep,2461093.6488,11.23,0.05,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
V0555 Cep 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:02.72 +65:09:50.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0545 Cep,2461093.6488,10.66,0.05,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
V0545 Cep 20260222.1488 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:06.02 +66:20:29.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
AX Cep,2461093.6488,10.29,0.05,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
AX Cep 20260222.1488 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:54.18 +70:13:15.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0579 Cep,2461093.6488,10.96,0.05,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
V0579 Cep 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:42.07 +67:49:31.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J212324.93+690857.9,2461093.6488,10.88,0.05,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 J212324.93+690857.9 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:25.12 +69:08:59.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0867 Cep,2461093.6488,10.90,0.05,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
V0867 Cep 20260222.1488 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:33.79 +71:18:24.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
BQ Cep,2461093.6488,11.10,0.05,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
BQ Cep 20260222.1488 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:26:55.72 +68:25:12.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0582 Cep,2461093.6488,10.79,0.05,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
V0582 Cep 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:28.22 +66:00:19.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211658.04+701543.9,2461093.6488,11.41,0.05,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
ASASSN-V J211658.04+701543.9 20260222.1488 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:58.28 +70:15:44.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211728.75+703050.9,2461093.6488,11.09,0.05,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 J211728.75+703050.9 20260222.1488 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:17:29.03 +70:30:50.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J212047.56+715956.6,2461093.6488,11.05,0.05,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
ASASSN-V J212047.56+715956.6 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:47.91 +71:59:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213838.42+730307.7,2461093.6488,11.03,0.05,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 J213838.42+730307.7 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:38.29 +73:03:03.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0566 Cep,2461093.6488,11.13,0.05,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
V0566 Cep 20260222.1488 11.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:10.31 +68:16:13.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
BT Cep,2461093.6488,10.05,0.05,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
BT Cep 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:31:29.97 +67:23:50.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0536 Cep,2461093.6488,10.29,0.05,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
V0536 Cep 20260222.1488 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:07.36 +65:31:18.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V1035 Cep,2461093.6488,9.99,0.05,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
V1035 Cep 20260222.1488 9.99CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:06.43 +74:35:21.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2120334+731801,2461093.6488,11.43,0.05,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
NSVS J2120334+731801 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:33.74 +73:17:58.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211617.08+715211.1,2461093.6488,11.38,0.05,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
ASASSN-V J211617.08+715211.1 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:17.89 +71:52:09.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0567 Cep,2461093.6488,10.80,0.05,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
V0567 Cep 20260222.1488 10.80CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:25.53 +67:58:26.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
CT Cep,2461093.6488,9.41,0.05,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
CT Cep 20260222.1488 9.41CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:12.20 +67:38:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
Vend21,2461093.6488,9.91,0.05,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
Vend21 20260222.1488 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:37.50 +71:31:11.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.38 20:35:53.84 +74:35:02.3
108.25499 19.59938 galactic Dra Second-epoch detections are separated by 0.2" and 4.1 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 2277788527650755072 | 20:35:55.75 +74:34:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2277788527650755072,2461093.6488,13.38,0.05,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 2277788527650755072 20260222.1488 13.38CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:35:53.84 +74:35:02.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2275596513783187712,2461093.6488,13.11,0.05,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
Gaia DR3 2275596513783187712 20260222.1488 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:26:22.96 +72:03:22.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.12 20:20:45.45 +70:42:26.9
104.12234 18.58183 galactic Dra Second-epoch detections are separated by 0.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2274675432276614656 | 20:20:46.53 +70:42:29.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2274675432276614656,2461093.6488,13.12,0.05,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
Gaia DR3 2274675432276614656 20260222.1488 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:20:45.45 +70:42:26.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.04 20:10:07.32 +69:37:48.8
102.66761 18.85593 galactic Dra Second-epoch detections are separated by 3.3" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2250495140060946432 | 20:10:08.73 +69:37:50.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2250495140060946432,2461093.6488,13.04,0.05,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
Gaia DR3 2250495140060946432 20260222.1488 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:10:07.32 +69:37:48.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.93 20:27:13.43 +65:44:51.3
100.00331 15.50738 galactic Cep Second-epoch detections are separated by 7.1" and 4.3 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 2246276077724082944 | 20:27:14.29 +65:44:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246276077724082944,2461093.6488,12.93,0.05,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 2246276077724082944 20260222.1488 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:13.43 +65:44:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.02 20:22:54.55 +71:21:28.8
104.80973 18.75405 galactic Dra Second-epoch detections are separated by 4.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2274729853805725184 | 20:22:54.42 +71:21:35.9 (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 2274729853805725184,2461093.6488,13.02,0.05,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 2274729853805725184 20260222.1488 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:22:54.55 +71:21:28.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.90 20:32:53.41 +64:50:36.0
99.55428 14.51745 galactic Cep Second-epoch detections are separated by 2.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2245405779911627648 | 20:32:53.13 +64:50:44.8 (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 2245405779911627648,2461093.6488,12.90,0.05,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 2245405779911627648 20260222.1488 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:32:53.41 +64:50:36.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.88 20:24:48.92 +68:31:58.8
102.34121 17.17486 galactic Dra Second-epoch detections are separated by 1.7" and 4.5 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 2250163877823289728 | 20:24:48.40 +68:31:44.1 (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 2250163877823289728,2461093.6488,12.88,0.05,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 2250163877823289728 20260222.1488 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:48.92 +68:31:58.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.76 20:51:44.53 +65:12:30.1
101.05687 13.11676 galactic Cep Second-epoch detections are separated by 0.5" and 5.1 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 2197579631145284480 | 20:51:44.74 +65:12:35.9 (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 2197579631145284480,2461093.6488,12.76,0.05,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 2197579631145284480 20260222.1488 12.76CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:51:44.53 +65:12:30.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.89 19:59:46.26 +73:19:43.4
105.82525 21.21164 galactic Dra Second-epoch detections are separated by 8.3" and 5.3 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 2287896269326197248 | 19:59:48.25 +73:20:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2287896269326197248,2461093.6488,12.89,0.05,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
Gaia DR3 2287896269326197248 20260222.1488 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:46.26 +73:19:43.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.77 20:19:38.33 +67:00:13.0
100.70580 16.81099 galactic Dra Second-epoch detections are separated by 3.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246590327593314944 | 20:19:40.39 +67:00:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246590327593314944,2461093.6488,12.77,0.05,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 2246590327593314944 20260222.1488 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:38.33 +67:00:13.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.78 20:23:23.83 +65:35:13.5
99.64492 15.75640 galactic Dra Second-epoch detections are separated by 1.2" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246258794775484288 | 20:23:24.26 +65:35:22.2 (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 2246258794775484288,2461093.6488,12.78,0.05,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
Gaia DR3 2246258794775484288 20260222.1488 12.78CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:23.83 +65:35:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2276816387573340032,2461093.6488,13.14,0.05,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
Gaia DR3 2276816387573340032 20260222.1488 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:08:08.20 +73:56:04.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.93 20:02:42.43 +71:34:15.7
104.21795 20.27404 galactic Dra Second-epoch detections are separated by 6.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251693715111391872 | 20:02:42.98 +71:33:58.8 (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 2251693715111391872,2461093.6488,12.93,0.05,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 2251693715111391872 20260222.1488 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:02:42.43 +71:34:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2197394092854213120,2461093.6488,13.00,0.05,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 2197394092854213120 20260222.1488 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:06:27.74 +64:59:50.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2222717185675638528,2461093.6488,13.02,0.05,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 2222717185675638528 20260222.1488 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:48.17 +67:56:56.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.78 20:24:15.33 +67:12:31.1
101.13044 16.53144 galactic Dra Second-epoch detections are separated by 5.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246675612761109632 | 20:24:17.44 +67:12:38.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246675612761109632,2461093.6488,12.78,0.05,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
Gaia DR3 2246675612761109632 20260222.1488 12.78CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:15.33 +67:12:31.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,12.80,0.05,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
target 20260222.1488 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:46.01 +65:10:07.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.66 20:41:48.08 +65:27:05.6
100.62033 14.09398 galactic Cep Second-epoch detections are separated by 6.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2245504117482140544 | 20:41:48.94 +65:27:09.5 (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 2245504117482140544,2461093.6488,12.66,0.05,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 2245504117482140544 20260222.1488 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:41:48.08 +65:27:05.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.64 20:43:09.53 +65:21:09.8
100.62269 13.92159 galactic Cep Second-epoch detections are separated by 1.8" and 5.2 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 2245312252704034048 | 20:43:10.58 +65:21:14.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2245312252704034048,2461093.6488,12.64,0.05,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
Gaia DR3 2245312252704034048 20260222.1488 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:43:09.53 +65:21:09.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.54 20:25:51.01 +66:05:13.4
100.22389 15.80699 galactic Dra Second-epoch detections are separated by 2.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246297002804962048 | 20:25:52.07 +66:05:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246297002804962048,2461093.6488,12.54,0.05,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
Gaia DR3 2246297002804962048 20260222.1488 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:51.01 +66:05:13.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.53 20:16:35.23 +67:18:38.9
100.82825 17.22131 galactic Dra Second-epoch detections are separated by 2.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2249610651674708992 | 20:16:36.37 +67:18:47.1 (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 2249610651674708992,2461093.6488,12.53,0.05,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 2249610651674708992 20260222.1488 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:35.23 +67:18:38.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.62 20:23:27.96 +66:01:10.9
100.03181 15.97709 galactic Dra Second-epoch detections are separated by 6.5" and 6.2 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 2246462994699850752 | 20:23:28.90 +66:01:16.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246462994699850752,2461093.6488,12.62,0.05,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
Gaia DR3 2246462994699850752 20260222.1488 12.62CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:27.96 +66:01:10.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.62 20:16:51.72 +68:34:54.6
102.00047 17.82685 galactic Dra Second-epoch detections are separated by 6.4" and 5.2 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 2249828183178306688 | 20:16:49.95 +68:34:47.5 (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 2249828183178306688,2461093.6488,12.62,0.05,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
Gaia DR3 2249828183178306688 20260222.1488 12.62CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:51.72 +68:34:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.56 20:54:48.06 +65:03:49.9
101.14363 12.77454 galactic Cep Second-epoch detections are separated by 3.1" and 5.5 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 2197582379924365056 | 20:54:49.40 +65:03:54.5 (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 2197582379924365056,2461093.6488,12.56,0.05,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
Gaia DR3 2197582379924365056 20260222.1488 12.56CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:54:48.06 +65:03:49.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.70 20:04:24.40 +73:03:41.1
105.71522 20.79552 galactic Dra Second-epoch detections are separated by 3.4" and 3.3 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 2287874863209261440 | 20:04:23.03 +73:03:36.9 (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 2287874863209261440,2461093.6488,12.70,0.05,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 2287874863209261440 20260222.1488 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:04:24.40 +73:03:41.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.59 20:19:23.66 +66:32:14.4
100.27367 16.59493 galactic Dra Second-epoch detections are separated by 8.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246538517405008512 | 20:19:24.56 +66:32:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246538517405008512,2461093.6488,12.59,0.05,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
Gaia DR3 2246538517405008512 20260222.1488 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:23.66 +66:32:14.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
WISE J202821.4+671453,2461093.6488,12.54,0.05,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
WISE J202821.4+671453 20260222.1488 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:28:21.38 +67:14:59.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.58 20:30:08.66 +66:47:01.5
101.07425 15.81829 galactic Cep Second-epoch detections are separated by 7.1" and 5.4 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 2246436091025167872 | 20:30:10.07 +66:47:00.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246436091025167872,2461093.6488,12.58,0.05,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 2246436091025167872 20260222.1488 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:30:08.66 +66:47:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,12.78,0.05,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
target 20260222.1488 12.78CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:28.57 +67:49:45.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.41 20:26:45.80 +67:26:55.8
101.47596 16.45188 galactic Dra Second-epoch detections are separated by 3.9" and 4.2 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 2246707567317842688 | 20:26:46.96 +67:26:57.9 (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 2246707567317842688,2461093.6488,12.41,0.05,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
Gaia DR3 2246707567317842688 20260222.1488 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:26:45.80 +67:26:55.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.52 20:14:11.83 +68:43:31.7
102.00817 18.10860 galactic Dra Second-epoch detections are separated by 5.3" and 4.2 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 2250020361492571008 | 20:14:09.60 +68:43:12.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2250020361492571008,2461093.6488,12.52,0.05,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
Gaia DR3 2250020361492571008 20260222.1488 12.52CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:14:11.83 +68:43:31.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.51 20:17:58.46 +67:19:00.6
100.90350 17.10837 galactic Dra Second-epoch detections are separated by 5.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2249599660856498816 | 20:18:00.02 +67:19:06.1 (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 2249599660856498816,2461093.6488,12.51,0.05,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 2249599660856498816 20260222.1488 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:17:58.46 +67:19:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.64 20:38:57.00 +68:14:26.9
102.82019 15.92261 galactic Dra Second-epoch detections are separated by 3.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246978386478524928 | 20:39:00.79 +68:14:44.2 (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 2246978386478524928,2461093.6488,12.64,0.05,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
Gaia DR3 2246978386478524928 20260222.1488 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:38:57.00 +68:14:26.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,12.85,0.05,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
target 20260222.1488 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:46.05 +69:03:54.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.60 20:19:06.67 +71:38:51.7
104.91923 19.15894 galactic Dra Second-epoch detections are separated by 1.5" and 4.3 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 2275499992980408704 | 20:19:08.09 +71:38:52.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2275499992980408704,2461093.6488,12.60,0.05,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 2275499992980408704 20260222.1488 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:06.67 +71:38:51.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.28 20:39:11.59 +65:31:13.9
100.51712 14.35463 galactic Cep Second-epoch detections are separated by 8.9" and 3.2 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 2245496146022827264 | 20:39:12.45 +65:31:16.9 (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 2245496146022827264,2461093.6488,12.28,0.05,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
Gaia DR3 2245496146022827264 20260222.1488 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:39:11.59 +65:31:13.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.22 20:18:53.99 +67:05:18.8
100.74426 16.91612 galactic Dra Second-epoch detections are separated by 3.2" and 5.3 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 2246591774999575936 | 20:18:55.25 +67:05:27.1 (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 2246591774999575936,2461093.6488,12.22,0.05,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
Gaia DR3 2246591774999575936 20260222.1488 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:18:53.99 +67:05:18.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.11 20:31:21.93 +67:03:47.4
101.38568 15.86959 galactic Cep Second-epoch detections are separated by 7.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246450212877843840 | 20:31:22.95 +67:03:49.5 (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 2246450212877843840,2461093.6488,12.11,0.05,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
Gaia DR3 2246450212877843840 20260222.1488 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:31:21.93 +67:03:47.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.06 20:21:45.72 +66:52:05.8
100.69531 16.56309 galactic Dra Second-epoch detections are separated by 5.7" and 5.1 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 2246570334522888832 | 20:21:46.84 +66:52:21.9 (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 2246570334522888832,2461093.6488,12.06,0.05,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 2246570334522888832 20260222.1488 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:21:45.72 +66:52:05.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2249788914295205248,2461093.6488,12.06,0.05,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 2249788914295205248 20260222.1488 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:15:05.12 +68:06:40.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.77 20:34:38.76 +66:26:22.1
101.03042 15.25587 galactic Cep Second-epoch detections are separated by 4.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246355002042750976 | 20:34:40.87 +66:26:25.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246355002042750976,2461093.6488,11.77,0.05,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 2246355002042750976 20260222.1488 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:34:38.76 +66:26:22.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.68 20:30:54.97 +66:38:55.6
100.99955 15.68093 galactic Cep Second-epoch detections are separated by 6.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246422656367494784 | 20:30:53.21 +66:38:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1956PMcCO..13a....B BD+66 1304
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 2246422656367494784,2461093.6488,11.68,0.05,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 2246422656367494784 20260222.1488 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:30:54.97 +66:38:55.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.69 20:32:05.58 +72:59:00.9
106.66546 18.98227 galactic Dra Second-epoch detections are separated by 2.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2276048035104262016 | 20:32:08.21 +72:58:57.9 (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 2276048035104262016,2461093.6488,11.69,0.05,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
Gaia DR3 2276048035104262016 20260222.1488 11.69CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:32:05.58 +72:59:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.26 20:26:08.99 +67:44:09.2
101.69830 16.65287 galactic Dra Second-epoch detections are separated by 1.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2247090712760496128 | 20:26:08.00 +67:44:05.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=11.089+/- (unrealisitic color!)
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 2247090712760496128,2461093.6488,11.26,0.05,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
Gaia DR3 2247090712760496128 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:26:08.99 +67:44:09.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.16 20:21:58.79 +68:45:18.2
102.40211 17.51037 galactic Dra Second-epoch detections are separated by 0.9" and 5.1 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 2250194427924688896 | 20:21:57.54 +68:45:15.7 (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: F2 1948UppAn...2d....S BD+68 1123
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 2250194427924688896,2461093.6488,11.16,0.05,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
Large-amplitude variable Gaia DR2 2250194427924688896 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:21:58.79 +68:45:18.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.12 20:27:14.16 +67:13:17.7
101.30022 16.29287 galactic Cep Second-epoch detections are separated by 2.6" and 4.5 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 2246649254544511616 | 20:27:16.51 +67:13:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1956PMcCO..13a....B AG+67 903
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 2246649254544511616,2461093.6488,11.12,0.05,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
Gaia DR3 2246649254544511616 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:14.16 +67:13:17.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.09 20:25:34.69 +67:29:45.2
101.45533 16.57316 galactic Dra Second-epoch detections are separated by 1.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246711312529496320 | 20:25:33.61 +67:29:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1956PMcCO..13a....B AG+67 900
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 2246711312529496320,2461093.6488,11.09,0.05,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 2246711312529496320 20260222.1488 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:34.69 +67:29:45.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
NGCA-V26,2461093.6488,10.69,0.05,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
NGCA-V26 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:38:14.68 +65:49:47.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.30 20:15:27.47 +70:03:17.2
103.29214 18.65146 galactic Dra Second-epoch detections are separated by 2.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2250621961854917248 | 20:15:30.74 +70:03:25.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0V 1948UppAn...2d....S BD+69 1096
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 2250621961854917248,2461093.6488,10.30,0.05,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
Gaia DR3 2250621961854917248 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:15:27.47 +70:03:17.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.62 20:18:26.15 +73:37:09.6
106.73029 20.14945 galactic Dra Second-epoch detections are separated by 2.3" and 4.3 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 2276319202159145984 | 20:18:27.97 +73:37:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1925sdsl.book.....L BD+73 903
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 2276319202159145984,2461093.6488,10.62,0.05,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
Gaia DR3 2276319202159145984 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:18:26.15 +73:37:09.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 10.77 20:38:42.14 +65:29:22.4
100.46082 14.37857 galactic Cep Second-epoch detections are separated by 1.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2245496420900685184 | 20:38:41.16 +65:29:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2245496420900685184,2461093.6488,10.77,0.05,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 2245496420900685184 20260222.1488 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:38:42.14 +65:29:22.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2245371866850109440,2461093.6488,10.86,0.05,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 2245371866850109440 20260222.1488 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:37:18.22 +64:54:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.19 20:21:40.33 +73:44:41.2
106.96352 20.01007 galactic Dra Second-epoch detections are separated by 3.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2276341153735421312 | 20:21:43.04 +73:44:39.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1948UppAn...2d....S BD+73 905
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 2276341153735421312,2461093.6488,11.19,0.05,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 2276341153735421312 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:21:40.33 +73:44:41.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.13 20:03:28.99 +72:51:43.8
105.49159 20.77183 galactic Dra Second-epoch detections are separated by 3.3" and 4.3 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 2275856513923115136 | 20:03:30.82 +72:51:46.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1948UppAn...2d....S BD+72 932
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 2275856513923115136,2461093.6488,11.13,0.05,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 2275856513923115136 20260222.1488 11.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:28.99 +72:51:43.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.22 20:13:19.13 +71:52:00.7
104.89520 19.66192 galactic Dra Second-epoch detections are separated by 4.6" and 4.3 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 2275544596218743168 | 20:13:20.74 +71:52:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1948UppAn...2d....S BD+71 1008
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 2275544596218743168,2461093.6488,11.22,0.05,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
Gaia DR3 2275544596218743168 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:19.13 +71:52:00.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.30 20:17:41.59 +72:28:52.0
105.63800 19.65583 galactic Dra Second-epoch detections are separated by 5.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275682653647151232 | 20:17:43.88 +72:28:48.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1948UppAn...2d....S BD+72 947
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 2275682653647151232,2461093.6488,11.30,0.05,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
Gaia DR3 2275682653647151232 20260222.1488 11.30CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:17:41.59 +72:28:52.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2251791704787463040,2461093.6488,11.23,0.05,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
Gaia DR3 2251791704787463040 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:01:44.40 +72:06:09.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.32 20:05:29.43 +71:39:22.0
104.40108 20.11319 galactic Dra Second-epoch detections are separated by 3.6" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251715018149218304 | 20:05:30.65 +71:39:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1948UppAn...2d....S BD+71 997
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 2251715018149218304,2461093.6488,11.32,0.05,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 2251715018149218304 20260222.1488 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:05:29.43 +71:39:22.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.27 20:19:29.80 +68:33:12.6
102.10003 17.60384 galactic Dra Second-epoch detections are separated by 1.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2250189033448596224 | 20:19:31.90 +68:33:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1948UppAn...2d....S BD+68 1119
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 2250189033448596224,2461093.6488,11.27,0.05,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 2250189033448596224 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:29.80 +68:33:12.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.41 20:13:45.72 +71:31:44.4
104.59524 19.47357 galactic Dra Second-epoch detections are separated by 4.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275521300315758464 | 20:13:48.38 +71:31:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1948UppAn...2d....S [S48] 108
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 2275521300315758464,2461093.6488,11.41,0.05,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
Gaia DR3 2275521300315758464 20260222.1488 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:45.72 +71:31:44.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.16 20:25:41.87 +64:47:58.4
99.08453 15.13458 galactic Dra Second-epoch detections are separated by 2.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2244664262398110464 | 20:25:41.36 +64:47:51.8 (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 2244664262398110464,2461093.6488,11.16,0.05,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
Gaia DR3 2244664262398110464 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:41.87 +64:47:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.43 20:27:02.28 +69:55:32.6
103.69629 17.72930 galactic Dra Second-epoch detections are separated by 7.0" and 4.3 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 2250385399353726336 | 20:27:04.14 +69:55:33.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1948UppAn...2d....S BD+69 1105
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 2250385399353726336,2461093.6488,11.43,0.05,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
Gaia DR3 2250385399353726336 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:02.28 +69:55:32.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.45 20:21:41.24 +71:57:48.9
105.31501 19.13819 galactic Dra Second-epoch detections are separated by 1.2" and 4.3 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 2275603832404726016 | 20:21:43.60 +71:57:51.4 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: F5 1948UppAn...2d....S [S48] 141
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 2275603832404726016,2461093.6488,11.45,0.05,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 2275603832404726016 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:21:41.24 +71:57:48.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.52 20:20:12.08 +69:06:04.5
102.63122 17.82302 galactic Dra Second-epoch detections are separated by 0.7" and 5.2 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 2250241084154276992 | 20:20:14.12 +69:06:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1948UppAn...2d....S [S48] 137
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 2250241084154276992,2461093.6488,11.52,0.05,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
Gaia DR3 2250241084154276992 20260222.1488 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:20:12.08 +69:06:04.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2250430719847274752,2461093.6488,11.49,0.05,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 2250430719847274752 20260222.1488 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:27.23 +69:14:32.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.56 20:12:20.08 +71:09:34.7
104.19231 19.40227 galactic Dra Second-epoch detections are separated by 2.6" and 5.2 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 2251493084301916800 | 20:12:22.72 +71:09:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1948UppAn...2d....S [S48] 103
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 2251493084301916800,2461093.6488,11.56,0.05,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
Gaia DR3 2251493084301916800 20260222.1488 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:20.08 +71:09:34.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.60 19:52:59.70 +73:19:19.9
105.61171 21.65524 galactic Dra Second-epoch detections are separated by 5.1" and 4.5 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 2287929147298696832 | 19:53:02.53 +73:19:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1948UppAn...2d....S BD+72 923
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 2287929147298696832,2461093.6488,11.60,0.05,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 2287929147298696832 20260222.1488 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:52:59.70 +73:19:19.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.51 20:29:20.30 +65:10:13.0
99.62283 15.01065 galactic Cep Second-epoch detections are separated by 0.6" and 5.1 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 2246179217618408448 | 20:29:19.36 +65:10:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1956PMcCO..13a....B AG+65 1031
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 2246179217618408448,2461093.6488,11.51,0.05,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 2246179217618408448 20260222.1488 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:29:20.30 +65:10:13.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.70 20:29:00.01 +73:26:37.9
106.96010 19.41155 galactic Dra Second-epoch detections are separated by 4.1" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2276125516314863232 | 20:29:02.50 +73:26:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1948UppAn...2d....S [S48] 150
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 2276125516314863232,2461093.6488,11.70,0.05,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 2276125516314863232 20260222.1488 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:29:00.01 +73:26:37.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.68 20:21:06.58 +71:07:52.6
104.52602 18.76674 galactic Dra Second-epoch detections are separated by 6.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2274702988786236800 | 20:21:09.69 +71:07:55.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1948UppAn...2d....S [S48] 139
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 2274702988786236800,2461093.6488,11.68,0.05,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 2274702988786236800 20260222.1488 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:21:06.58 +71:07:52.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.65 20:23:17.51 +71:23:23.0
104.85488 18.74348 galactic Dra Second-epoch detections are separated by 8.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2274730029900513536 | 20:23:18.98 +71:23:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1948UppAn...2d....S [S48] 142
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 2274730029900513536,2461093.6488,11.65,0.05,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
Gaia DR3 2274730029900513536 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:17.51 +71:23:23.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.74 20:44:40.42 +65:35:08.2
100.91202 13.93142 galactic Cep Second-epoch detections are separated by 2.3" and 5.3 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 2245696463297426688 | 20:44:45.64 +65:34:52.8 (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 2245696463297426688,2461093.6488,11.74,0.05,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 2245696463297426688 20260222.1488 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:40.42 +65:35:08.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.88 20:23:04.05 +72:42:26.1
106.05487 19.41435 galactic Dra Second-epoch detections are separated by 4.4" and 5.3 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 2275703372569617920 | 20:23:06.70 +72:42:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1948UppAn...2d....S [S48] 143
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 2275703372569617920,2461093.6488,11.88,0.05,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 2275703372569617920 20260222.1488 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:04.05 +72:42:26.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.82 20:14:35.94 +71:38:05.2
104.72721 19.46481 galactic Dra Second-epoch detections are separated by 5.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275527931745443968 | 20:14:38.55 +71:38:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1948UppAn...2d....S [S48] 113
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 2275527931745443968,2461093.6488,11.82,0.05,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 2275527931745443968 20260222.1488 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:14:35.94 +71:38:05.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.91 20:14:32.15 +72:40:17.3
105.69814 19.95399 galactic Dra Second-epoch detections are separated by 5.1" and 5.1 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 2275873448977078272 | 20:14:33.57 +72:40:20.1 (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 2275873448977078272,2461093.6488,11.91,0.05,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 2275873448977078272 20260222.1488 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:14:32.15 +72:40:17.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.80 20:01:55.27 +72:51:00.7
105.42798 20.87112 galactic Dra Second-epoch detections are separated by 5.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2287865105044088704 | 20:01:56.70 +72:51:01.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1948UppAn...2d....S BD+72 929
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 2287865105044088704,2461093.6488,11.80,0.05,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
Gaia DR3 2287865105044088704 20260222.1488 11.80CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:01:55.27 +72:51:00.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J202458.90+651121.2,2461093.6488,11.78,0.05,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
ASASSN-V J202458.90+651121.2 20260222.1488 11.78CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:59.79 +65:11:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.80 20:12:40.38 +70:15:02.5
103.35547 18.95256 galactic Dra Second-epoch detections are separated by 1.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251378808108091776 | 20:12:44.17 +70:15:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1948UppAn...2d....S BD+69 1094
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 2251378808108091776,2461093.6488,11.80,0.05,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
Gaia DR3 2251378808108091776 20260222.1488 11.80CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:40.38 +70:15:02.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.90 19:55:02.31 +73:16:00.1
105.61800 21.49836 galactic Dra Second-epoch detections are separated by 1.4" and 4.4 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 2287916232334122368 | 19:55:05.44 +73:15:56.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1948UppAn...2d....S BD+72 925
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 2287916232334122368,2461093.6488,11.90,0.05,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 2287916232334122368 20260222.1488 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:02.31 +73:16:00.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.92 20:03:47.27 +71:52:53.9
104.55578 20.33119 galactic Dra Second-epoch detections are separated by 2.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251773601503275776 | 20:03:48.56 +71:52:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1948UppAn...2d....S [S48] 87
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 2251773601503275776,2461093.6488,11.92,0.05,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 2251773601503275776 20260222.1488 11.92CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:47.27 +71:52:53.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.99 20:10:23.34 +72:20:54.4
105.24056 20.08271 galactic Dra Second-epoch detections are separated by 5.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275780578901283328 | 20:10:24.82 +72:20:58.1 (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 2275780578901283328,2461093.6488,11.99,0.05,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 2275780578901283328 20260222.1488 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:10:23.34 +72:20:54.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.12 20:28:27.06 +74:01:30.0
107.47023 19.74046 galactic Dra Second-epoch detections are separated by 2.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2276431627223508864 | 20:28:30.15 +74:01:22.9 (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 2276431627223508864,2461093.6488,12.12,0.05,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
Gaia DR3 2276431627223508864 20260222.1488 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:28:27.06 +74:01:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.20 20:18:42.22 +73:49:31.7
106.93317 20.23063 galactic Dra Second-epoch detections are separated by 8.4" and 5.1 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 2276370054571922816 | 20:18:44.57 +73:49:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1948UppAn...2d....S [S48] 130
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 2276370054571922816,2461093.6488,12.20,0.05,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
Gaia DR3 2276370054571922816 20260222.1488 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:18:42.22 +73:49:31.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.21 20:22:34.18 +73:11:29.5
106.48308 19.68459 galactic Dra Second-epoch detections are separated by 8.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2276101705015491200 | 20:22:37.50 +73:11:25.5 (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 2276101705015491200,2461093.6488,12.21,0.05,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
Gaia DR3 2276101705015491200 20260222.1488 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:22:34.18 +73:11:29.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.28 20:09:32.12 +73:25:53.3
106.24338 20.62391 galactic Dra Second-epoch detections are separated by 7.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275990650044293504 | 20:09:33.58 +73:25:55.2 (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 2275990650044293504,2461093.6488,12.28,0.05,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
Gaia DR3 2275990650044293504 20260222.1488 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:09:32.12 +73:25:53.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.21 19:59:16.99 +73:33:21.4
106.03274 21.33596 galactic Dra Second-epoch detections are separated by 3.9" and 4.4 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 2288040820745309696 | 19:59:15.84 +73:33:29.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2288040820745309696,2461093.6488,12.21,0.05,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
Gaia DR3 2288040820745309696 20260222.1488 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:16.99 +73:33:21.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.21 19:59:13.12 +73:33:35.1
106.03448 21.34168 galactic Dra Second-epoch detections are separated by 5.8" and 5.1 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 2288040820745309696 | 19:59:15.84 +73:33:29.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2288040820745309696,2461093.6488,12.21,0.05,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
Gaia DR3 2288040820745309696 20260222.1488 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:13.12 +73:33:35.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.20 20:21:11.54 +70:20:32.7
103.80739 18.36889 galactic Dra Second-epoch detections are separated by 8.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2250641654279850240 | 20:21:14.21 +70:20:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2250641654279850240,2461093.6488,12.20,0.05,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
Gaia DR3 2250641654279850240 20260222.1488 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:21:11.54 +70:20:32.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2251336133312803712,2461093.6488,12.19,0.05,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 2251336133312803712 20260222.1488 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:36.79 +70:17:56.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.31 20:23:48.88 +73:30:27.0
106.82193 19.76234 galactic Dra Second-epoch detections are separated by 8.4" and 4.3 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 2276299857626534784 | 20:23:51.45 +73:30:23.8 (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 2276299857626534784,2461093.6488,12.31,0.05,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
Gaia DR3 2276299857626534784 20260222.1488 12.31CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:48.88 +73:30:27.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.24 20:03:01.62 +72:46:36.9
105.39374 20.76616 galactic Dra Second-epoch detections are separated by 5.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275854280539954048 | 20:03:03.02 +72:46:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1948UppAn...2d....S [S48] 80
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 2275854280539954048,2461093.6488,12.24,0.05,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
Gaia DR3 2275854280539954048 20260222.1488 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:01.62 +72:46:36.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.21 20:18:40.09 +68:52:26.1
102.35224 17.82879 galactic Dra Second-epoch detections are separated by 7.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2250213050903355776 | 20:18:42.19 +68:52:33.2 (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 2250213050903355776,2461093.6488,12.21,0.05,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
Gaia DR3 2250213050903355776 20260222.1488 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:18:40.09 +68:52:26.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.37 20:18:53.53 +73:13:04.2
106.37088 19.92978 galactic Dra Second-epoch detections are separated by 3.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275917326362979712 | 20:18:55.91 +73:13:02.5 (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 2275917326362979712,2461093.6488,12.37,0.05,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
Gaia DR3 2275917326362979712 20260222.1488 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:18:53.53 +73:13:04.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.37 19:57:26.92 +73:21:20.6
105.77947 21.37476 galactic Dra Second-epoch detections are separated by 1.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2287938325645925376 | 19:57:25.38 +73:21:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2287938325645925376,2461093.6488,12.37,0.05,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
Gaia DR3 2287938325645925376 20260222.1488 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:26.92 +73:21:20.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.32 20:30:45.05 +64:53:06.6
99.46038 14.72982 galactic Cep Second-epoch detections are separated by 2.6" and 5.3 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 2245404783480220800 | 20:30:45.74 +64:53:10.9 (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 2245404783480220800,2461093.6488,12.32,0.05,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 2245404783480220800 20260222.1488 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:30:45.05 +64:53:06.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.40 20:20:55.73 +72:14:23.8
105.53964 19.32470 galactic Dra Second-epoch detections are separated by 0.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275663721431359104 | 20:20:58.86 +72:14:23.1 (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 2275663721431359104,2461093.6488,12.40,0.05,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 2275663721431359104 20260222.1488 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:20:55.73 +72:14:23.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.41 20:12:46.83 +69:49:54.9
102.96980 18.74703 galactic Dra Second-epoch detections are separated by 8.1" and 4.1 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 2250519402332036864 | 20:12:49.58 +69:49:57.9 (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 2250519402332036864,2461093.6488,12.41,0.05,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
Gaia DR3 2250519402332036864 20260222.1488 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:46.83 +69:49:54.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.55 20:23:41.89 +73:45:15.7
107.04603 19.89105 galactic Dra Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2276330536576265344 | 20:23:43.93 +73:45:03.9 (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 2276330536576265344,2461093.6488,12.55,0.05,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
Gaia DR3 2276330536576265344 20260222.1488 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:41.89 +73:45:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.53 20:16:11.53 +69:46:08.0
103.06010 18.45828 galactic Dra Second-epoch detections are separated by 2.1" and 4.5 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 2250510159562489344 | 20:16:15.06 +69:46:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2250510159562489344,2461093.6488,12.53,0.05,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 2250510159562489344 20260222.1488 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:11.53 +69:46:08.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2245294213841286528,2461093.6488,12.49,0.05,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 2245294213841286528 20260222.1488 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:24.26 +65:08:24.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.64 20:12:02.76 +72:28:59.7
105.42896 20.03255 galactic Dra Second-epoch detections are separated by 5.1" and 5.4 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 2275777207349564800 | 20:12:05.46 +72:28:57.8 (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 2275777207349564800,2461093.6488,12.64,0.05,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
Gaia DR3 2275777207349564800 20260222.1488 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:02.76 +72:28:59.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.65 20:16:12.43 +69:46:10.5
103.06141 18.45748 galactic Dra Second-epoch detections are separated by 5.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2250510159562489344 | 20:16:15.06 +69:46:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2250510159562489344,2461093.6488,12.65,0.05,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
Gaia DR3 2250510159562489344 20260222.1488 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:12.43 +69:46:10.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,12.94,0.05,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
target 20260222.1488 12.94CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:42.03 +68:15:09.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.62 20:23:34.74 +72:19:48.6
105.72817 19.19391 galactic Dra Second-epoch detections are separated by 6.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275641726901834112 | 20:23:34.47 +72:20:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2275641726901834112,2461093.6488,12.62,0.05,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
Gaia DR3 2275641726901834112 20260222.1488 12.62CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:34.74 +72:19:48.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.69 20:02:41.06 +71:33:47.3
104.20953 20.27229 galactic Dra Second-epoch detections are separated by 4.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251693715111391872 | 20:02:42.98 +71:33:58.8 (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 2251693715111391872,2461093.6488,12.69,0.05,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
Gaia DR3 2251693715111391872 20260222.1488 12.69CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:02:41.06 +71:33:47.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.86 20:03:44.65 +73:12:47.0
105.84018 20.90354 galactic Dra Second-epoch detections are separated by 4.7" and 4.2 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 2287879914090793472 | 20:03:47.33 +73:12:58.8 (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 2287879914090793472,2461093.6488,12.86,0.05,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 2287879914090793472 20260222.1488 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:44.65 +73:12:47.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2244956320174552704,2461093.6488,12.57,0.05,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
Gaia DR3 2244956320174552704 20260222.1488 12.57CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:20:13.06 +65:50:49.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2152533+690352,2461093.6488,13.03,0.05,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
NSVS J2152533+690352 20260222.1488 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:52.86 +69:03:51.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.89 19:56:20.86 +72:45:39.5
105.16002 21.21034 galactic Dra Second-epoch detections are separated by 6.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2287851361147945728 | 19:56:22.26 +72:45:41.5 (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 2287851361147945728,2461093.6488,12.89,0.05,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
Gaia DR3 2287851361147945728 20260222.1488 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:56:20.86 +72:45:39.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.71 20:03:31.19 +70:29:17.7
103.20988 19.74532 galactic Dra Second-epoch detections are separated by 1.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251364583176164736 | 20:03:33.19 +70:29:19.2 (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 2251364583176164736,2461093.6488,12.71,0.05,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 2251364583176164736 20260222.1488 12.71CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:31.19 +70:29:17.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0523 Cep,2461093.6488,13.13,0.05,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
V0523 Cep 20260222.1488 13.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:35:41.14 +64:40:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.88 20:53:57.19 +65:32:08.1
101.46728 13.13631 galactic Cep Second-epoch detections are separated by 4.2" and 5.4 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 2197613170548463488 | 20:53:55.59 +65:32:02.8 (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 2197613170548463488,2461093.6488,12.88,0.05,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 2197613170548463488 20260222.1488 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:53:57.19 +65:32:08.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.94 19:59:38.86 +73:28:15.3
105.96066 21.27775 galactic Dra Second-epoch detections are separated by 3.3" and 4.3 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 2287945747349552640 | 19:59:42.65 +73:28:17.1 (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 2287945747349552640,2461093.6488,12.94,0.05,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 2287945747349552640 20260222.1488 12.94CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:38.86 +73:28:15.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.01 19:55:32.44 +73:14:48.3
105.61357 21.45726 galactic Dra Second-epoch detections are separated by 8.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2287915373340672512 | 19:55:36.49 +73:14:41.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2287915373340672512,2461093.6488,13.01,0.05,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 2287915373340672512 20260222.1488 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:32.44 +73:14:48.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.99 20:03:26.43 +70:16:18.6
103.00012 19.65652 galactic Dra Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251334582827798400 | 20:03:29.14 +70:16:19.1 (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 2251334582827798400,2461093.6488,12.99,0.05,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 2251334582827798400 20260222.1488 12.99CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:26.43 +70:16:18.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.97 20:24:21.08 +64:54:57.6
99.10778 15.31764 galactic Dra Second-epoch detections are separated by 1.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2244677078580576000 | 20:24:23.05 +64:54:59.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2244677078580576000,2461093.6488,12.97,0.05,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 2244677078580576000 20260222.1488 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:21.08 +64:54:57.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2245516070372819072,2461093.6488,13.07,0.05,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 2245516070372819072 20260222.1488 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:41:55.67 +65:44:21.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.10 20:54:52.49 +65:53:47.2
101.81873 13.28509 galactic Cep Second-epoch detections are separated by 7.9" and 6.2 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 2245751816836073856 | 20:54:49.47 +65:54:06.5 (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 2245751816836073856,2461093.6488,13.10,0.05,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 2245751816836073856 20260222.1488 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:54:52.49 +65:53:47.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2245285280309108096,2461093.6488,13.04,0.05,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
Gaia DR3 2245285280309108096 20260222.1488 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:41:39.76 +65:06:35.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.00 20:22:44.01 +65:30:16.7
99.53456 15.77172 galactic Dra Second-epoch detections are separated by 3.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2244757617807621120 | 20:22:45.12 +65:30:21.2 (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 2244757617807621120,2461093.6488,13.00,0.05,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 2244757617807621120 20260222.1488 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:22:44.01 +65:30:16.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2215543+650632,2461093.6488,13.45,0.05,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
NSVS J2215543+650632 20260222.1488 13.45CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:54.07 +65:06:37.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.28 20:05:25.34 +73:26:03.6
106.10937 20.88899 galactic Dra Second-epoch detections are separated by 2.1" and 4.5 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 2287982576691952896 | 20:05:22.56 +73:26:03.2 (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 2287982576691952896,2461093.6488,13.28,0.05,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
Gaia DR3 2287982576691952896 20260222.1488 13.28CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:05:25.34 +73:26:03.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.09 20:29:02.10 +65:03:54.2
99.51348 14.98013 galactic Cep Second-epoch detections are separated by 1.1" and 5.3 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 2245422032067852928 | 20:29:03.12 +65:03:55.1 (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 2245422032067852928,2461093.6488,13.09,0.05,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 2245422032067852928 20260222.1488 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:29:02.10 +65:03:54.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J204952.14+743133.6,2461093.6488,13.49,0.05,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 J204952.14+743133.6 20260222.1488 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:49:53.98 +74:31:35.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
FI Cep,2461093.6488,13.25,0.05,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
FI Cep 20260222.1488 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:10.40 +67:20:30.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.26 19:56:54.77 +72:55:15.2
105.33512 21.23615 galactic Dra Second-epoch detections are separated by 2.9" and 5.1 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 2287859882363833344 | 19:56:58.71 +72:55:06.8 (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 2287859882363833344,2461093.6488,13.26,0.05,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
Gaia DR3 2287859882363833344 20260222.1488 13.26CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:56:54.77 +72:55:15.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.20 20:19:26.45 +71:38:05.7
104.92077 19.13004 galactic Dra Second-epoch detections are separated by 5.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275499202706426496 | 20:19:28.44 +71:38:08.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2275499202706426496,2461093.6488,13.20,0.05,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
Gaia DR3 2275499202706426496 20260222.1488 13.20CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:26.45 +71:38:05.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.16 20:16:27.82 +66:48:30.4
100.36591 16.98206 galactic Dra Second-epoch detections are separated by 8.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2249559524385330432 | 20:16:29.48 +66:48:21.9 (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 2249559524385330432,2461093.6488,13.16,0.05,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
Gaia DR3 2249559524385330432 20260222.1488 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:27.82 +66:48:30.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.18 20:23:24.73 +65:42:34.7
99.75419 15.81936 galactic Dra Second-epoch detections are separated by 6.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246261990232113024 | 20:23:27.98 +65:42:35.2 (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 2246261990232113024,2461093.6488,13.18,0.05,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
Gaia DR3 2246261990232113024 20260222.1488 13.18CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:24.73 +65:42:34.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.41 20:07:44.38 +69:25:31.1
102.37391 18.94635 galactic Dra Second-epoch detections are separated by 4.4" and 4.4 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 2250862480022572288 | 20:07:44.12 +69:25:54.2 (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 2250862480022572288,2461093.6488,13.41,0.05,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
Gaia DR3 2250862480022572288 20260222.1488 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:07:44.38 +69:25:31.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.62 20:28:47.46 +65:52:11.8
100.20000 15.43797 galactic Cep Second-epoch detections are separated by 2.7" and 5.1 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 2246237491738037504 | 20:28:46.70 +65:52:06.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246237491738037504,2461093.6488,13.62,0.05,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
Gaia DR3 2246237491738037504 20260222.1488 13.62CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:28:47.46 +65:52:11.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J202646.52+645038.5,2461093.6488,13.62,0.05,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
ASASSN-V J202646.52+645038.5 20260222.1488 13.62CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:26:47.73 +64:50:46.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2246014+670720,2461093.6488,14.14,0.05,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
NSVS J2246014+670720 20260222.1488 14.14CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:46:00.15 +67:07:22.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,13.75,0.05,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
target 20260222.1488 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:28:06.49 +65:41:43.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2255581+672036,2461093.6488,14.44,0.05,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
NSVS J2255581+672036 20260222.1488 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:55:56.82 +67:20:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J220042.82+703757.0,2461093.6488,12.87,0.05,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
ASASSN-V J220042.82+703757.0 20260222.1488 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:42.55 +70:37:56.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J212626.54+695654.4,2461093.6488,13.04,0.05,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 J212626.54+695654.4 20260222.1488 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:27.43 +69:56:56.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0595 Cep,2461093.6488,11.77,0.05,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
V0595 Cep 20260222.1488 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:30.84 +69:17:46.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J210024.76+715024.8,2461093.6488,11.66,0.05,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 J210024.76+715024.8 20260222.1488 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:25.44 +71:50:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J214252.13+695515.1,2461093.6488,12.40,0.05,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 J214252.13+695515.1 20260222.1488 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:52.00 +69:55:15.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.46 20:19:19.83 +66:04:25.8
99.85426 16.36443 galactic Dra Second-epoch detections are separated by 3.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246474642651112704 | 20:19:21.91 +66:04:22.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2246474642651112704,2461093.6488,12.46,0.05,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 2246474642651112704 20260222.1488 12.46CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:19.83 +66:04:25.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0858 Cep,2461093.6488,12.99,0.05,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
V0858 Cep 20260222.1488 12.99CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:45.12 +72:57:46.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.70 21:17:35.63 +70:04:34.1
106.51458 14.36668 galactic Cep Second-epoch detections are separated by 1.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2270844802485579392 | 21:17:35.40 +70:04:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.441+/-0.028 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2270844802485579392,2461093.6488,11.70,0.05,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 2270844802485579392 20260222.1488 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:17:35.63 +70:04:34.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0608 Cep,2461093.6488,11.84,0.05,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
V0608 Cep 20260222.1488 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:34.44 +67:08:08.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,13.13,0.05,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
target 20260222.1488 13.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:23.95 +69:04:10.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211815.16+723308.2,2461093.6488,12.55,0.05,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
ASASSN-V J211815.16+723308.2 20260222.1488 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:15.27 +72:33:05.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V1051 Cep,2461093.6488,12.26,0.05,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
V1051 Cep 20260222.1488 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:08.63 +68:02:45.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
GSC 04467-00632,2461093.6488,11.07,0.05,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
GSC 04467-00632 20260222.1488 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:49.30 +70:18:31.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J210454.20+670807.9,2461093.6488,13.11,0.05,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
ASASSN-V J210454.20+670807.9 20260222.1488 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:54.54 +67:08:11.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J210426.06+671605.0,2461093.6488,12.59,0.05,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
ASASSN-V J210426.06+671605.0 20260222.1488 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:26.49 +67:16:07.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213324.34+665744.2,2461093.6488,13.13,0.05,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
ASASSN-V J213324.34+665744.2 20260222.1488 13.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:24.17 +66:57:46.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J203240.85+685504.6,2461093.6488,13.44,0.05,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
ASASSN-V J203240.85+685504.6 20260222.1488 13.44CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:32:42.06 +68:55:05.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,13.16,0.05,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
target 20260222.1488 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:53.46 +69:42:29.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2226072345407267840,2461093.6488,13.37,0.05,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
Gaia DR3 2226072345407267840 20260222.1488 13.37CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:34:35.47 +69:06:22.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.45 21:38:44.92 +70:56:59.3
108.43275 13.72642 galactic Cep Second-epoch detections are separated by 2.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:38:44.92 +70:56:59.3 (user input) | T | P | (position from user input) J-Ks=1.448+/-0.032 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6488,13.45,0.05,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
target 20260222.1488 13.45CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:44.92 +70:56:59.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0492 Cep,2461093.6488,13.10,0.05,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
V0492 Cep 20260222.1488 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:03.52 +66:39:14.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J214637.40+671312.4,2461093.6488,13.18,0.05,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
ASASSN-V J214637.40+671312.4 20260222.1488 13.18CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:37.15 +67:13:12.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J210824.91+744335.1,2461093.6488,12.70,0.05,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 J210824.91+744335.1 20260222.1488 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:08:25.58 +74:43:29.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.82 21:32:05.49 +68:03:34.6
105.95685 12.03342 galactic Cep Second-epoch detections are separated by 4.5" and 5.1 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 2222170453516295424 | 21:32:13.00 +68:03:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2222170453516295424,2461093.6488,12.82,0.05,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 2222170453516295424 20260222.1488 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:05.49 +68:03:34.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.97 20:41:11.29 +65:24:06.7
100.54044 14.11699 galactic Cep Second-epoch detections are separated by 1.0" and 5.2 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 2245502330775698816 | 20:41:10.68 +65:24:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2245502330775698816,2461093.6488,11.97,0.05,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 2245502330775698816 20260222.1488 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:41:11.29 +65:24:06.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
EL Cep,2461093.6488,12.51,0.05,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
EL Cep 20260222.1488 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:22.69 +69:11:06.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J220523.43+644143.0,2461093.6488,12.86,0.05,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 J220523.43+644143.0 20260222.1488 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:23.09 +64:41:46.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2102066+732546,2461093.6488,11.96,0.05,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
NSVS J2102066+732546 20260222.1488 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:07.89 +73:25:45.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2056120+733332,2461093.6488,12.79,0.05,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
NSVS J2056120+733332 20260222.1488 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:56:13.48 +73:33:30.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0978 Cep,2461093.6488,13.36,0.05,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
V0978 Cep 20260222.1488 13.36CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:30.50 +66:26:04.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0631 Cep,2461093.6488,12.47,0.05,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
V0631 Cep 20260222.1488 12.47CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:43.17 +65:03:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2157344+650209,2461093.6488,12.55,0.05,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
NSVS J2157344+650209 20260222.1488 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:34.51 +65:02:12.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J223212.62+671808.4,2461093.6488,13.43,0.05,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 J223212.62+671808.4 20260222.1488 13.43CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:32:12.21 +67:18:10.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 3382200,2461093.6488,12.97,0.05,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 3382200 20260222.1488 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:22.06 +65:57:05.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211214.01+713237.9,2461093.6488,11.90,0.05,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 J211214.01+713237.9 20260222.1488 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:12:14.44 +71:32:36.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0363 Cep,2461093.6488,12.84,0.05,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
V0363 Cep 20260222.1488 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:31.45 +71:48:57.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213915.14+654333.7,2461093.6488,13.09,0.05,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 J213915.14+654333.7 20260222.1488 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:14.96 +65:43:35.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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,2461093.6488,12.36,0.05,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 20260222.1488 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:58:42.10 +70:03:25.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2240374+663035,2461093.6488,12.39,0.05,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
NSVS J2240374+663035 20260222.1488 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:40:35.93 +66:30:39.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J220734.66+700818.8,2461093.6488,13.31,0.05,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
ZTF J220734.66+700818.8 20260222.1488 13.31CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:35.06 +70:08:20.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V1038 Cep,2461093.6488,11.31,0.05,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
V1038 Cep 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:12:13.98 +71:03:50.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213909.47+732930.0,2461093.6488,9.94,0.05,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
ASASSN-V J213909.47+732930.0 20260222.1488 9.94CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:09.36 +73:29:25.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213934.18+692838.4,2461093.6488,12.79,0.05,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
ASASSN-V J213934.18+692838.4 20260222.1488 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:33.81 +69:28:37.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2141448+665243,2461093.6488,12.16,0.05,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
NSVS J2141448+665243 20260222.1488 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:44.97 +66:52:46.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J220612.20+720220.1,2461093.6488,13.41,0.05,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
ASASSN-V J220612.20+720220.1 20260222.1488 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:11.90 +72:02:18.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.46 21:20:47.01 +68:08:38.4
105.25884 12.84211 galactic Cep Second-epoch detections are separated by 0.3" and 4.5 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 2222311946918387328 | 21:20:46.93 +68:08:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.431+/-0.031 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2222311946918387328,2461093.6488,11.46,0.05,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 2222311946918387328 20260222.1488 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:47.01 +68:08:38.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J214031.67+740808.2,2461093.6488,9.91,0.05,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 J214031.67+740808.2 20260222.1488 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:31.74 +74:08:03.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211424.49+675908.4,2461093.6488,11.43,0.05,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 J211424.49+675908.4 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:14:24.69 +67:59:10.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J215246.69+725837.1,2461093.6488,11.96,0.05,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
ASASSN-V J215246.69+725837.1 20260222.1488 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:46.39 +72:58:34.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J215318.15+660450.3,2461093.6488,12.96,0.05,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
ASASSN-V J215318.15+660450.3 20260222.1488 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:17.88 +66:04:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 1367511,2461093.6488,12.85,0.05,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
NSVS 1367511 20260222.1488 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:34.71 +68:48:26.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213255.52+690001.4,2461093.6488,13.09,0.05,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 J213255.52+690001.4 20260222.1488 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:55.57 +69:00:00.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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,2461093.6488,12.04,0.05,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
VARIABLE_NAME 20260222.1488 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:21.82 +69:58:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J215804.25+662810.9,2461093.6488,12.13,0.05,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
ASASSN-V J215804.25+662810.9 20260222.1488 12.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:03.96 +66:28:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J205949.86+713109.0,2461093.6488,13.15,0.05,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
ASASSN-V J205949.86+713109.0 20260222.1488 13.15CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:59:50.59 +71:31:07.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
FQ Cep,2461093.6488,12.41,0.05,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
FQ Cep 20260222.1488 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:55:10.51 +67:02:00.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211614.18+691225.9,2461093.6488,12.82,0.05,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 J211614.18+691225.9 20260222.1488 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:14.25 +69:12:27.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 21039+6758,2461093.6488,11.36,0.05,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
IRAS 21039+6758 20260222.1488 11.36CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:36.71 +68:10:12.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0598 Dra,2461093.6488,9.76,0.05,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
V0598 Dra 20260222.1488 9.76CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:35:39.96 +73:00:07.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213628.06+684341.9,2461093.6488,11.73,0.05,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 J213628.06+684341.9 20260222.1488 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:28.07 +68:43:42.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J210012.07+665443.0,2461093.6488,11.46,0.05,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
ASASSN-V J210012.07+665443.0 20260222.1488 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:12.28 +66:54:45.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213128.98+653527.0,2461093.6488,11.72,0.05,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 J213128.98+653527.0 20260222.1488 11.72CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:28.87 +65:35:29.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 1233980,2461093.6488,12.22,0.05,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
NSVS 1233980 20260222.1488 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:55.97 +73:05:42.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J220300.84+712611.5,2461093.6488,13.30,0.05,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
ASASSN-V J220300.84+712611.5 20260222.1488 13.30CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:00.53 +71:26:10.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2022022+652512,2461093.6488,12.98,0.05,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 J2022022+652512 20260222.1488 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:22:03.05 +65:25:14.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0665 Cep,2461093.6488,12.79,0.05,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
V0665 Cep 20260222.1488 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:24:58.64 +69:20:32.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213319.60+654325.1,2461093.6488,12.71,0.05,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
ASASSN-V J213319.60+654325.1 20260222.1488 12.71CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:19.56 +65:43:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
ZALD J20571172+7142580,2461093.6488,11.83,0.05,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
ZALD J20571172+7142580 20260222.1488 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:57:12.42 +71:42:56.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211646.19+674014.6,2461093.6488,12.35,0.05,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 J211646.19+674014.6 20260222.1488 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:46.32 +67:40:14.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0574 Cep,2461093.6488,10.80,0.05,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
V0574 Cep 20260222.1488 10.80CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:32.29 +67:52:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2151128+675611,2461093.6488,12.73,0.05,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 J2151128+675611 20260222.1488 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:12.86 +67:56:12.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J212749.13+653959.8,2461093.6488,13.21,0.05,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 J212749.13+653959.8 20260222.1488 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:49.06 +65:40:02.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213943.95+651529.1,2461093.6488,12.10,0.05,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
ASASSN-V J213943.95+651529.1 20260222.1488 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:42.82 +65:15:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V1037 Cep,2461093.6488,10.68,0.05,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
V1037 Cep 20260222.1488 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:08:48.28 +73:26:07.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.26 22:02:06.31 +70:50:22.6
109.85173 12.40303 galactic Cep Second-epoch detections are separated by 1.6" and 3.9 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 | target | 22:02:06.31 +70:50:22.6 (user input) | T | P | (position from user input) J-Ks=1.396+/-0.041 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6488,13.26,0.05,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
target 20260222.1488 13.26CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:06.31 +70:50:22.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2120155+713520,2461093.6488,13.03,0.05,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
NSVS J2120155+713520 20260222.1488 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:16.23 +71:35:19.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.53 20:03:07.88 +71:38:47.7
104.30601 20.27629 galactic Dra Second-epoch detections are separated by 3.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2251717526410083840 | 20:03:07.24 +71:38:49.5 (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 2251717526410083840,2461093.6488,12.53,0.05,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 2251717526410083840 20260222.1488 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:07.88 +71:38:47.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2137198+694805,2461093.6488,12.64,0.05,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
NSVS J2137198+694805 20260222.1488 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:17.20 +69:47:52.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,12.01,0.05,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
target 20260222.1488 12.01CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:10.23 +70:26:17.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211850.53+702829.2,2461093.6488,12.09,0.05,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 J211850.53+702829.2 20260222.1488 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:50.66 +70:28:29.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
BK Cep,2461093.6488,11.39,0.05,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
BK Cep 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:26.36 +68:18:10.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 V1299,2461093.6488,12.74,0.05,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 V1299 20260222.1488 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:35.53 +67:10:49.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 11.57 20:06:28.13 +71:56:42.9
104.71348 20.17164 galactic Dra Second-epoch detections are separated by 1.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2275744295017337216 | 20:06:29.46 +71:56:43.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1948UppAn...2d....S BD+71 999
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 2275744295017337216,2461093.6488,11.57,0.05,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
Gaia DR3 2275744295017337216 20260222.1488 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:06:28.13 +71:56:42.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2243075+660854,2461093.6488,13.24,0.05,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
NSVS J2243075+660854 20260222.1488 13.24CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:43:06.17 +66:08:59.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J212259.02+682108.4,2461093.6488,12.03,0.05,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 J212259.02+682108.4 20260222.1488 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:59.08 +68:21:09.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 3395915,2461093.6488,13.03,0.05,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
NSVS 3395915 20260222.1488 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:27.70 +66:26:45.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2219520+720116,2461093.6488,12.29,0.05,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 J2219520+720116 20260222.1488 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:19:51.58 +72:01:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2140040+703243,2461093.6488,11.87,0.05,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
NSVS J2140040+703243 20260222.1488 11.87CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:03.24 +70:32:41.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J205607.54+713339.7,2461093.6488,11.25,0.05,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 J205607.54+713339.7 20260222.1488 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:56:08.33 +71:33:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V1046 Cep,2461093.6488,11.59,0.05,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
V1046 Cep 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:12.31 +74:00:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2223798486639960704,2461093.6488,13.14,0.05,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
Gaia DR3 2223798486639960704 20260222.1488 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:21.59 +68:53:19.2 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2147365+662832,2461093.6488,12.73,0.05,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 J2147365+662832 20260222.1488 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:36.52 +66:28:37.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J214951.12+683119.0,2461093.6488,12.97,0.05,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 J214951.12+683119.0 20260222.1488 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:51.61 +68:31:23.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J220133.06+703412.4,2461093.6488,13.54,0.05,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
ASASSN-V J220133.06+703412.4 20260222.1488 13.54CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:32.82 +70:34:12.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.17 22:20:41.64 +69:23:35.9
110.29991 10.30719 galactic Cep Second-epoch detections are separated by 3.7" and 4.5 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 2226270360578179456 | 22:20:42.40 +69:24:16.1 (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 2226270360578179456,2461093.6488,13.17,0.05,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
Gaia DR3 2226270360578179456 20260222.1488 13.17CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:20:41.64 +69:23:35.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2222192+642940,2461093.6488,13.13,0.05,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
NSVS J2222192+642940 20260222.1488 13.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:22:18.59 +64:29:43.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 1361619,2461093.6488,12.31,0.05,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
NSVS 1361619 20260222.1488 12.31CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:55.66 +70:25:49.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J215747.42+670426.7,2461093.6488,12.69,0.05,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 J215747.42+670426.7 20260222.1488 12.69CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:47.10 +67:04:28.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0630 Cep,2461093.6488,11.19,0.05,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
V0630 Cep 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:26.71 +67:59:46.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J220548.56+732903.2,2461093.6488,12.46,0.05,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
ASASSN-V J220548.56+732903.2 20260222.1488 12.46CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:47.84 +73:28:59.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2048268+670502,2461093.6488,11.57,0.05,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 J2048268+670502 20260222.1488 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:48:27.25 +67:05:04.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,12.81,0.05,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
target 20260222.1488 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:03.34 +65:41:36.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J215453.45+721041.9,2461093.6488,12.84,0.05,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
ASASSN-V J215453.45+721041.9 20260222.1488 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:52.97 +72:10:40.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2104157+674246,2461093.6488,11.57,0.05,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 J2104157+674246 20260222.1488 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:16.01 +67:42:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J214614.17+645354.3,2461093.6488,12.89,0.05,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
ASASSN-V J214614.17+645354.3 20260222.1488 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:14.01 +64:53:57.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J211657.94+724518.9,2461093.6488,13.39,0.05,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 J211657.94+724518.9 20260222.1488 13.39CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:58.14 +72:45:17.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0573 Cep,2461093.6488,12.13,0.05,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
V0573 Cep 20260222.1488 12.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:16.39 +66:40:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J214139.76+711004.8,2461093.6488,10.54,0.05,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
ASASSN-V J214139.76+711004.8 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:39.71 +71:10:04.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,13.29,0.05,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
target 20260222.1488 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:11:51.02 +65:10:27.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 2224739874749380352,2461093.6488,13.51,0.05,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 2224739874749380352 20260222.1488 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:16.19 +71:49:10.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J214755.04+681230.9,2461093.6488,12.74,0.05,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 J214755.04+681230.9 20260222.1488 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:55.08 +68:12:32.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 22107+7042,2461093.6488,12.34,0.05,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
IRAS 22107+7042 20260222.1488 12.34CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:50.28 +70:56:52.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.77 20:35:36.69 +65:09:04.9
99.98420 14.45189 galactic Cep Second-epoch detections are separated by 0.6" and 5.2 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 2245392821991252608 | 20:35:36.35 +65:09:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2245392821991252608,2461093.6488,12.77,0.05,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 2245392821991252608 20260222.1488 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:35:36.69 +65:09:04.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0602 Cep,2461093.6488,12.11,0.05,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
V0602 Cep 20260222.1488 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:36.34 +66:45:26.6 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J215542.35+672845.3,2461093.6488,12.03,0.05,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 J215542.35+672845.3 20260222.1488 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:41.98 +67:28:45.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0548 Cep,2461093.6488,11.86,0.05,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
V0548 Cep 20260222.1488 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:00.12 +65:39:26.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2113202+702404,2461093.6488,12.64,0.05,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
NSVS J2113202+702404 20260222.1488 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:13:19.28 +70:24:05.7 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J213912.18+682527.2,2461093.6488,8.50,0.05,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 J213912.18+682527.2 20260222.1488 8.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:12.14 +68:25:29.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2155251+691116,2461093.6488,13.02,0.05,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
NSVS J2155251+691116 20260222.1488 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:24.66 +69:11:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J220432.24+692122.7,2461093.6488,12.05,0.05,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
ASASSN-V J220432.24+692122.7 20260222.1488 12.05CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:31.85 +69:21:23.4 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J214007.19+692756.6,2461093.6488,12.80,0.05,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
ASASSN-V J214007.19+692756.6 20260222.1488 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:06.91 +69:27:57.8 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
FR Cep,2461093.6488,12.20,0.05,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
FR Cep 20260222.1488 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:55:46.97 +68:12:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 1391152,2461093.6488,12.89,0.05,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
NSVS 1391152 20260222.1488 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:45:07.94 +69:58:34.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J210214.22+700718.8,2461093.6488,12.41,0.05,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
ASASSN-V J210214.22+700718.8 20260222.1488 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:14.59 +70:07:19.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J210741.52+673428.9,2461093.6488,13.46,0.05,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
ASASSN-V J210741.52+673428.9 20260222.1488 13.46CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:07:41.94 +67:34:32.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
target,2461093.6488,13.27,0.05,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
target 20260222.1488 13.27CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:47.77 +68:11:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0851 Cep,2461093.6488,13.13,0.05,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
V0851 Cep 20260222.1488 13.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:22.78 +70:19:28.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
V0598 Cep,2461093.6488,11.79,0.05,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
V0598 Cep 20260222.1488 11.79CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:21.70 +67:18:10.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J210645.62+700418.9,2461093.6488,12.04,0.05,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 J210645.62+700418.9 20260222.1488 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:06:45.86 +70:04:20.3 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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
BM Cep,2461093.6488,11.12,0.05,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
BM Cep 20260222.1488 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:44.98 +66:59:41.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J212502.71+731551.7,2461093.6488,13.62,0.05,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
ASASSN-V J212502.71+731551.7 20260222.1488 13.62CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:25:02.83 +73:15:49.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 13.08 22:13:23.83 +70:51:08.0
110.61992 11.86089 galactic Cep Second-epoch detections are separated by 0.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2229646956488042112 | 22:13:24.32 +70:51:08.1 (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 2229646956488042112,2461093.6488,13.08,0.05,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 2229646956488042112 20260222.1488 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:23.83 +70:51:08.0 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J212021.39+681803.6,2461093.6488,12.13,0.05,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
ASASSN-V J212021.39+681803.6 20260222.1488 12.13CV 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:21.40 +68:18:04.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1488 2461093.6488 12.84 21:36:29.20 +68:33:35.1
106.61031 12.11534 galactic Cep Second-epoch detections are separated by 0.4" and 4.4 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 2223686473892139520 | 21:36:29.24 +68:33:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.577+/-0.030 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2223686473892139520,2461093.6488,12.84,0.05,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 2223686473892139520 20260222.1488 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:29.20 +68:33:35.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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 J2129100+661302,2461093.6488,11.52,0.05,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
NSVS J2129100+661302 20260222.1488 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:10.18 +66:13:07.9 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20_00sec_-14_90C_LIGHT_0078_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: 2461032.60255554 23.12.2025 02:27:30.799 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
First image: 2461032.60255554 23.12.2025 02:27:30.799 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
Last image: 2461093.64913514 22.02.2026 03:34:35.276 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 155
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
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: 23 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): 15596
Objects passed selection criteria: 15541
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 12542
Average stars matched: 12148.2 (96.8605 %)
Memory usage VmPeak: 121284 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 Sun Feb 22 01:32:34 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: 2461032.60255554 23.12.2025 02:27:30.799 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
First image: 2461032.60255554 23.12.2025 02:27:30.799 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
Last image: 2461093.64913514 22.02.2026 03:34:35.276 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 866
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 124 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): 104513
Objects passed selection criteria: 104286
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: 79235.8
Average stars matched: 75430.8 (95.1979 %)
Memory usage VmPeak: 1934884 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 Sun Feb 22 01:39:59 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:
Cep-04-Q2b1x1
#######################################
########### Starting Cep-04-Q2b1x1 ###########
Processing Cep-04-Q2b1x1
server tau has sufficient free disk space available: 1075626 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1075626 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.png' -> 'transient_report/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits_preview.png'
Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
renamed 'Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.png' -> 'transient_report/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits_preview.png'
Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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= 691.3715
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 692.6447
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1538.1816
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 617.2037
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1538.2644
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 616.2504
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.22483
INFO: SECOND_EPOCH__SD_ratio= 0.002
----------------------------------------------
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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat to cache
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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: 2461093.64852988
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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits exists and is non-empty
Saving wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits to local_wcs_cache/
'wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits'
wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits'
wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits exists and is non-empty
Saving wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits to local_wcs_cache/
'wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits' -> 'local_wcs_cache/wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits'
wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits exists and is non-empty
Saving wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits to local_wcs_cache/
'wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits' -> 'local_wcs_cache/wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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 21:36:17.587 +69:59:17.38
Second-epoch image center 21:36:00.556 +70:00:02.57
Angular distance between the image centers 0.03 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 21:36:17.587 +69:59:17.38
Second-epoch image center 21:36:04.514 +69:59:46.74
Angular distance between the image centers 0.02 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 21:36:00.556 +70:00:02.57
Second-epoch second image center 21:36:04.514 +69:59:46.74
Angular distance between the image centers 0.00715 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits &> /tmp/tmp.9y80d7ZzNo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits &> /tmp/tmp.WZKAC2XVt5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits &> /tmp/tmp.XoRkElcXiD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits &> /tmp/tmp.i95z2sSxWA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits and wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits and wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits and wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat
The reference image (wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits) and catalog (wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat) found
'wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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 8972 out of 15980 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.913946
a=0.000000 b=1.000000 c=22.913946
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.18
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 146 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
2.1 pix Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
3.8 pix Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
3.8 pix Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
Limiting magnitude estimates:
15.2 mag. Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
15.2 mag. Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
14.1 mag. Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
14.1 mag. Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.7 (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.9y80d7ZzNo (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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1418, passed=15980
Got 15980 stars (including 14536 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 15980 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits -region wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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.WZKAC2XVt5 (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/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1408, passed=16079
Got 16079 stars (including 14653 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 16079 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits -region wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.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.XoRkElcXiD (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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=800, passed=9213
Got 9213 stars (including 8410 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat
util/solve_plate_with_UCAC5 got 9213 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 970 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: 0.98"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.00"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.01"
Estimated accuracy of the plate solution: 1.04"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits -region wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.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.i95z2sSxWA (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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=812, passed=9225
Got 9225 stars (including 8410 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat
util/solve_plate_with_UCAC5 got 9225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 969 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: 1.00"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.01"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.01"
Estimated accuracy of the plate solution: 1.04"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits -region wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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 Cep-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out08464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20406.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out20991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21138.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out21187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21192.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21206.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out21232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21233.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out21247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21306.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out21349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21394.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out21411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21446.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_local.txt__out01201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04539.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out04891.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out06582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07352.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out09514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13820.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out20990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20994.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out21336.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out21369.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 65s
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: 40s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20961_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20961_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:34:42.93 +72:48:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 0.852 2275292327017216640 308.67807451740 +72.80658070366 10.7391 10.2950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20962_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20962_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:32:08.17 +72:58:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.397 2276048035104262016 308.03419880370 +72.98276074941 10.6527 10.2578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20963_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20963_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:03.99 +69:55:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.413 2250385395056533888 306.76722995689 +69.92600016024 10.3703 10.0796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20964_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20964_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:57.35 +68:50:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 3.045 2250256511676830208 306.99118295868 +68.83581832485 10.2177 9.8298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20965_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20965_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:43.87 +69:39:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 0.679 2250537338115432704 305.43317227800 +69.65361557030 10.0993 9.5965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20966_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20966_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:53:17.93 +74:43:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 4.810 2277088310542452736 313.32955733926 +74.72466394289 10.5273 10.0811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20967_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20967_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:37.35 +66:48:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 2.545 2246439252121085696 307.40742013537 +66.80677347273 10.2411 9.5078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20969_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20969_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:08:41.86 +73:06:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 4.295 2275956741279254016 302.17043101778 +73.11509426537 9.8299 9.4649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20970_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20970_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:13.79 +65:57:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 2.788 2246239656401641600 307.30928684911 +65.95437785809 9.7227 9.2527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20971_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20971_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:06.76 +66:54:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 5.399 2246619709466626560 306.53171171305 +66.91189611988 9.7509 9.3195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20972_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20972_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:07.27 +67:44:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 4.238 2247090712760496128 306.53335315445 +67.73493791722 9.8886 9.5692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20973_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 20973_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 20975_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20975_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:10.54 +68:52:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 0.610 2250177900893766144 306.29438650736 +68.87758693834 9.8294 9.4031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20976_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20976_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:57.70 +68:45:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 1.211 2250194427927556736 305.48972565293 +68.75435850938 9.8835 9.5588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20977_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20977_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:15.75 +67:13:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 4.524 2246649254544511616 306.81879260023 +67.22377475320 9.7922 9.4508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20978_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20978_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:38.81 +69:17:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 2.542 2250331110966406528 306.66368453180 +69.28587683298 10.0706 9.6341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20979_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20979_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:17:44.33 +72:28:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 3.233 2275682653647151232 304.43284746236 +72.48010349703 10.0867 9.6498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20980_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20980_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:53.73 +68:09:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 4.556 2250128835186908672 305.47708618197 +68.16339078601 9.9467 9.5148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20981_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20981_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:33:54.30 +72:38:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 1.851 2275266174961462016 308.47783517366 +72.64440901352 10.1778 9.6974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20982_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20982_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 20983_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20983_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:30:41.04 +65:44:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.92, MAG_FAINT_SEARCH_LIMIT=11.90)GAIADR2_OUTPUT=# 1.603 2246220552386986752 307.67054337367 +65.73787393301 9.4644 9.0141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20984_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20984_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:32.78 +67:29:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 4.787 2246711312529496320 306.39001713648 +67.49547932243 9.6866 9.3613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20985_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20985_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:37.75 +67:08:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 5.042 2246683103184013568 305.41080039866 +67.14915675200 9.5475 9.1635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20986_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20986_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:43.64 +73:44:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 2.811 2276341153735421312 305.42932240099 +73.74439556394 10.0204 9.6046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20987_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20987_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:08.73 +69:18:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 1.015 2250284656600145152 306.78649496452 +69.31561027328 9.7381 9.2767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20990_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 20990_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 20991_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20991_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:35.27 +67:28:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 2.315 2246717119324994688 305.64855288862 +67.47164472320 9.4289 9.0279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20992_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20992_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 20993_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20993_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:11.77 +66:07:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 3.199 2245587985305202944 309.79946665834 +66.12840601972 9.2279 8.9299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20994_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 20994_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 20996_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20996_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:11.36 +67:47:14.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20997_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20997_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:39.07 +67:00:39.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20998_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20998_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 20999_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20999_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 21000_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21000_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 21001_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21001_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:26.80 +68:17:07.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21002_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21002_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:44:57.27 +74:43:19.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21003_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21003_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 21004_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21004_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 21006_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21006_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:19:22.33 +64:52:24.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21011_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21011_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:25.73 +73:54:35.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21015_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21015_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:13:19.31 +72:53:50.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21021_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21021_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:51.73 +72:46:59.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21024_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21024_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:56:45.14 +72:18:37.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21031_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21031_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:13:16.21 +71:06:28.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21036_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21036_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:27.72 +70:39:33.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21042_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21042_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:11:38.71 +73:58:49.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21049_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21049_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:49:54.94 +64:59:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.39, MAG_FAINT_SEARCH_LIMIT=10.37)GAIADR2_OUTPUT=# 1.073 2197569430597680512 312.47850490835 +64.98684155439 8.3664 7.4376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21050_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21050_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:41:22.59 +65:02:18.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21052_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21052_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:11:25.55 +71:59:11.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21056_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21056_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:56:41.89 +72:56:17.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21062_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21062_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:10:03.44 +70:50:17.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21064_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21064_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:15:12.16 +72:08:08.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21065_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21065_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:17:02.51 +72:52:49.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21072_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21072_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:07.94 +70:08:43.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21074_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21074_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21075_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21075_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:17:42.43 +71:08:34.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21095_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21095_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:35.87 +72:22:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 0.949 2275810025197169664 301.14963378632 +72.38026953467 9.1334 8.6437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21105_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21105_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21107_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21107_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21109_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21109_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 21110_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21110_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:12.69 +65:51:18.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21112_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21112_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21113_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21113_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21116_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21116_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21118_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21118_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21129_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21129_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21135_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21135_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21137_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21137_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 21138_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21138_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:18:26.68 +73:37:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)GAIADR2_OUTPUT=# 5.464 2276319202159145984 304.61651779163 +73.61911488364 9.3859 9.0104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21141_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21141_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 21153_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21153_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:57:28.91 +72:19:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 5.771 2263811089162557440 299.37561995089 +72.33163255009 9.4045 9.1107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21162_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21162_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:06.39 +65:16:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)GAIADR2_OUTPUT=# 3.047 2245477248166645376 310.02542269135 +65.27187465220 9.4023 8.0955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21165_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21165_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21172_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21172_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21185_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21185_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21187_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21187_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:38:22.22 +64:57:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.76, MAG_FAINT_SEARCH_LIMIT=11.74)GAIADR2_OUTPUT=# 2.667 2245373103800750976 309.59368373845 +64.96613180754 9.7012 8.8223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21192_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21192_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:46:24.92 +65:03:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 2.454 2245248240511367168 311.60303304315 +65.05362994750 9.8251 8.7371 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21193_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21193_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:22.89 +64:58:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 1.814 2245382582790254336 308.84533044180 +64.97230910633 9.6352 8.8605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21194_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21194_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 21198_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21198_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21200_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21200_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 21202_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21202_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:19.48 +65:32:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 5.489 2246246871946229120 306.07888972584 +65.54096836555 9.4274 8.6044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21206_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21206_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:09:28.73 +70:40:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 2.851 2251450482522422528 302.36877049263 +70.67911743647 9.4981 9.0773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21209_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21209_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21210_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21210_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:37:17.37 +64:54:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.66, MAG_FAINT_SEARCH_LIMIT=11.64)GAIADR2_OUTPUT=# 1.566 2245371866850109440 309.32321799504 +64.90972437371 9.1914 8.9121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21232_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21232_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:03:30.00 +72:51:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 3.621 2275856513923115136 300.87840849357 +72.86280658488 9.8050 9.4312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21233_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21233_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:00:26.76 +67:59:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 3.230 2223089988835993472 330.11270911054 +67.99569777673 10.0613 8.5933 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21243_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21243_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:57:52.88 +72:11:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 3.916 2263800403283937280 299.47365417515 +72.19727655459 9.8329 9.4764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21244_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21244_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:05:29.85 +71:39:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 3.773 2251715018149218304 301.37768972085 +71.65664872719 10.0247 9.6684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21245_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21245_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21247_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21247_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:01:45.31 +72:06:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 3.773 2251791739147130368 300.44209946248 +72.10268882349 9.8305 9.4790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21258_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21258_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21263_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21263_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21267_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21267_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21292_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21292_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:12:13.95 +71:03:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 2.249 2271696438662817280 318.05633337860 +71.06417308530 10.5153 9.0181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21300_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21300_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:28.53 +71:56:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 4.425 2275744295017337216 301.62275003186 +71.94551572222 10.2641 9.9287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21302_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21302_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:02:39.83 +71:04:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.587 2251664646772609408 300.66374838073 +71.06951933014 10.2056 9.7231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21306_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21306_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:31.14 +64:51:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 4.677 2244666976817560320 306.88220954759 +64.86263331655 9.9104 9.3124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21307_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21307_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:57:26.22 +67:09:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 0.708 2219652537530210304 329.35938184490 +67.15636579730 10.7001 9.2597 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21309_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21309_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:59:29.97 +72:14:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 4.289 2251797172283829632 299.87869728713 +72.23368745956 10.1592 9.7047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21318_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21318_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:32.48 +65:04:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 3.867 2245392001656834560 308.88744607541 +65.06968387244 10.2079 9.4258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21336_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21336_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21348_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21348_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21349_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21349_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:24.30 +65:03:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 3.411 2245468830030591616 309.85232343945 +65.05113791937 10.3492 9.5278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21351_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21351_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:29:10.18 +66:13:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 3.870 2221136397190368896 322.29265103272 +66.21784595942 10.8790 9.4897 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21356_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21356_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:33.72 +64:55:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 0.773 2245276449856159744 310.13999468080 +64.92870929154 10.3496 9.3524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21358_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21358_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21361_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21361_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:00:58.06 +71:20:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 5.764 2251684437981890688 300.24691920460 +71.34260145018 10.2158 9.7284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21362_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21362_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21369_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21369_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21394_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21394_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:50:30.87 +69:17:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 2.385 2223086862099819776 327.63022308690 +69.29598718962 10.9922 9.3616 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21395_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21395_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:04:15.98 +67:42:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 2.831 2269981170461142656 316.06517170127 +67.71286848222 10.8048 9.4348 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21411_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21411_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:48:27.15 +67:05:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 4.804 2246063081705345920 312.11142143099 +67.08342557200 10.9573 9.5291 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21414_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21414_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:52:21.69 +67:18:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.815 2222668875882710528 328.09120833756 +67.30234278907 11.0620 9.6251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21417_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21417_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:48:02.03 +72:06:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.674 2272840965844218112 327.00958286383 +72.10620015319 11.3509 10.0643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21419_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21419_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:51:15.31 +72:40:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 5.199 2230089651656403072 342.81852937886 +72.68153282522 10.5805 9.1590 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21446_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21446_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:21:07.79 +70:50:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 4.259 2229609023338485632 335.28390606667 +70.84805567809 12.1732 11.2635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21495_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21495_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:48:14.37 +71:17:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.600 2226866635178780544 342.06123680600 +71.29761088982 11.9479 11.1050 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 05005_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 05005_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 20663_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20663_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:36:28.02 +68:43:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 0.851 2223735642677957632 324.11691498088 +68.72829902058 11.2336 9.9047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20081_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 20081_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 08987_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 08987_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13820_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 13820_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13640_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 13640_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 06582_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 06582_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 10137_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 10137_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 08358_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 08358_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 04584_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 04584_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07352_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 07352_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14942_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 14942_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06658_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 06658_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06287_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 06287_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04359_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 04359_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02873_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 02873_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09514_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 09514_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08675_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 08675_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15399_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 15399_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01201_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 01201_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02773_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 02773_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04539_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 04539_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20406_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 20406_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:32:12.29 +74:00:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 5.157 2274181712899271552 323.05059535697 +74.01206127316 11.0394 9.6565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10005_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 10005_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10309_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 10309_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04891_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 04891_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08464_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 08464_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:08:26.32 +68:18:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 2.533 2220112580064336384 332.11145044306 +68.30264387966 10.7214 9.3874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 14s
make_report_in_HTML.sh TOTAL: 119s
Prepared the HTML report for the field Cep-04-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 ####
21:00:06.43 +74:35:21.9
21:20:33.74 +73:17:58.7
21:38:38.29 +73:03:03.8
21:20:47.91 +71:59:54.6
21:16:17.89 +71:52:09.3
21:57:33.79 +71:18:24.7
21:20:37.50 +71:31:11.0
21:51:16.86 +71:04:29.5
21:17:29.03 +70:30:50.9
21:26:54.18 +70:13:15.4
21:16:58.28 +70:15:44.2
22:26:55.72 +68:25:12.9
21:23:25.12 +69:08:59.2
22:31:29.97 +67:23:50.0
21:35:42.56 +68:39:08.6
21:39:10.31 +68:16:13.8
21:39:25.53 +67:58:26.2
21:44:42.07 +67:49:31.0
21:46:12.20 +67:38:13.5
21:28:06.02 +66:20:29.5
21:32:02.72 +65:09:50.2
21:45:28.22 +66:00:19.7
21:19:07.36 +65:31:18.3
22:32:58.85 +66:54:43.5
20:26:21.56 +66:28:43.2
20:39:55.26 +73:32:07.8
20:30:15.79 +66:44:12.1
20:29:33.52 +67:02:15.7
19:56:26.86 +73:36:58.5
20:01:16.49 +72:54:15.9
20:22:25.21 +70:03:41.4
20:27:22.59 +72:44:39.6
20:36:46.02 +65:25:39.3
20:14:32.22 +70:50:20.6
20:25:04.46 +72:56:16.7
20:25:26.70 +73:13:53.6
20:30:34.81 +65:27:11.2
20:13:51.87 +72:28:28.7
20:25:40.31 +64:47:48.0
20:03:01.33 +72:37:10.6
20:20:36.24 +66:09:01.0
19:54:15.53 +73:23:22.0
20:37:00.01 +65:15:24.6
20:23:50.97 +69:35:48.2
20:20:57.02 +73:41:09.9
23:00:10.28 +70:02:27.3
20:03:44.77 +71:36:25.5
20:36:38.77 +68:17:39.4
20:04:23.02 +71:45:46.6
20:49:42.41 +72:15:49.0
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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat to cache
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
Creating symlink local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
Creating symlink local_wcs_cache/wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits exists and is non-empty
wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits exists and is non-empty
wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits exists and is non-empty
wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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 21:36:17.587 +69:59:17.38
Second-epoch image center 21:36:00.556 +70:00:02.57
Angular distance between the image centers 0.03 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 21:36:17.587 +69:59:17.38
Second-epoch image center 21:36:04.514 +69:59:46.74
Angular distance between the image centers 0.02 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 21:36:00.556 +70:00:02.57
Second-epoch second image center 21:36:04.514 +69:59:46.74
Angular distance between the image centers 0.00715 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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits &> /tmp/tmp.yOodE7ntBB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits &> /tmp/tmp.gQHj4pDte1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits &> /tmp/tmp.vHTC3UB3Cf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits &> /tmp/tmp.XxBQl5Eqbj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits and wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits and wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits and wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat
The reference image (wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits) and catalog (wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat) found
'wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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 9234 out of 112243 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.769686
a=0.000000 b=1.000000 c=22.769686
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 785 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
2.0 pix Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
3.6 pix Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
3.6 pix Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
Limiting magnitude estimates:
15.4 mag. Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
15.3 mag. Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
14.4 mag. Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
14.4 mag. Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yOodE7ntBB (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/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=10961, passed=112199
Got 112199 stars (including 101038 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 112199 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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: 0.38"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits -region wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.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.gQHj4pDte1 (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/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=10917, passed=111746
Got 111746 stars (including 100624 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 111746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 968 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits -region wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.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.vHTC3UB3Cf (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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=5571, passed=48145
Got 48145 stars (including 42534 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat
util/solve_plate_with_UCAC5 got 48145 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 969 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: 0.91"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.94"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.94"
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits -region wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-33-42_20.00sec_-14.90C_LIGHT_0078.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.XxBQl5Eqbj (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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=48, blended=5634, passed=48077
Got 48077 stars (including 42417 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat
util/solve_plate_with_UCAC5 got 48077 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.96"
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: 0.96"
Estimated accuracy of the plate solution: 0.96"
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_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cep-04-Q2b1x1_213641_TTUQ2b1x1_27058_FIgC3WCh/Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits -region wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079.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 Cep-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out108509.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out133389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out15680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out16262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out28710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out131864.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out133942.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out06638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99736.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 286s
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: 158s
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Considering the candidate 131693_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131693_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 23:14:42.89 +72:18:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 1.485 2228295386120077696 348.67820502341 +72.30966087931 13.5485 13.0204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131694_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131694_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 23:10:59.66 +71:56:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.535 2228281294330343552 347.74720893286 +71.94863175608 13.4035 12.5746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131697_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131697_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:41:12.02 +64:34:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.911 2211560784785657856 340.30131847549 +64.57054981816 13.2277 12.5758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131702_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131702_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:07:05.66 +69:12:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.409 2223303843846630784 331.77574334706 +69.21567758202 13.7151 12.9924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131704_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131704_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:41.34 +72:31:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 4.274 2276011373263274496 307.16933165913 +72.52666221369 12.7994 12.2817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131712_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131712_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 131713_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131713_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:42:12.71 +64:06:43.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 131715_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131715_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:40:17.39 +64:15:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.593 2211365312235230848 340.07262832771 +64.26063306457 12.9002 12.3998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131719_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131719_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:46:47.54 +66:31:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.200 2245940795397182976 311.69783948575 +66.53031341999 12.3439 11.7659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131721_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131721_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 131724_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131724_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:09:53.22 +71:54:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 2.780 2275729485970154752 302.46930098240 +71.91089284384 12.1779 11.5946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131726_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131726_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:15:52.06 +65:39:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 3.209 2218667306392979840 333.96488293295 +65.65094783974 13.6307 12.9495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131728_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131728_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:19.83 +65:10:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 5.301 2245393719643799168 308.83219811215 +65.18443380969 11.6748 11.1690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131729_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131729_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131738_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131738_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:22.41 +69:09:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.854 2271249457124116608 310.09330048439 +69.15173673326 12.5242 11.9706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131741_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131741_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:15.30 +65:40:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.732 2245524355368114688 309.81204236982 +65.67001126840 11.8151 11.3330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131743_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131743_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 131746_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131746_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:03.76 +69:37:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.471 2250360759123044736 307.01726414374 +69.61738951065 12.3627 11.8528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131747_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131747_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:30.45 +74:01:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.889 2276249722471891200 307.37832235822 +74.02795159773 12.0772 11.5566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131748_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131748_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131752_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131752_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131753_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131753_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131754_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131754_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:24.37 +65:14:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 5.180 2245395540709982336 308.85425977284 +65.24179665615 11.7404 11.1644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131755_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131755_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131756_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131756_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131762_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131762_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131763_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131763_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131765_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131765_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:51.99 +67:02:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.130 2246766043295040000 308.96993128687 +67.04861546620 11.8515 11.3529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131768_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131768_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:49:41.67 +65:06:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 5.167 2245610667030640000 312.42455621692 +65.10357500740 11.8683 11.4290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131770_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131770_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131771_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131771_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:47:27.25 +68:13:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.797 2270948225298270848 311.86397192340 +68.21725080831 12.3004 11.8500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131772_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131772_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:51:53.34 +65:14:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 4.847 2197580146542518784 312.97537284576 +65.24237607781 12.0846 11.6038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131774_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131774_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:30:10.52 +66:40:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.380 2246434613556426624 307.54581278933 +66.68420857444 11.8252 11.3267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131775_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131775_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:54.99 +68:59:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.507 2250180748453726336 306.22982150899 +69.00060839430 11.7326 11.2019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131776_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131776_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131777_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131777_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:34.58 +68:19:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.749 2250132408599879808 305.64765419576 +68.32237659564 11.7308 11.1682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131778_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131778_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:44.13 +73:14:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.410 2276107855408883840 305.93358988714 +73.23914326711 11.9121 11.3862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131780_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131780_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131781_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131781_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:24.80 +66:48:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.286 2246745088151804160 309.85564528189 +66.80913089813 11.8883 11.2987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131782_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131782_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:14:31.11 +65:53:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.592 2218686131230698368 333.63039482977 +65.88725542964 12.9560 12.0059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131784_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131784_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131785_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131785_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:33:50.10 +65:27:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.569 2245460171377900544 308.45849203099 +65.45967184436 11.4960 10.9949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131786_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131786_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:33.71 +65:52:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.627 2246279307539580288 306.88986923895 +65.86770104779 11.7915 10.8278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131787_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131787_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131788_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131788_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131789_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131789_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131790_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131790_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:12.74 +70:43:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.073 2274640144824716032 307.05456719873 +70.72166382184 11.8257 11.3395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131792_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131792_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131793_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131793_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 131794_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131794_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:17:51.80 +71:47:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.844 2275552017922090240 304.46834627341 +71.79407954453 11.7713 11.3076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131795_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131795_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 131796_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131796_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:16:42.67 +72:10:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 3.576 2275578474920739584 304.18027644689 +72.18038874102 11.6224 11.1411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131797_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131797_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:10:21.38 +71:36:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.031 2275536452960362624 302.58939153190 +71.60813865186 11.7242 11.2901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131798_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131798_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:28.75 +70:24:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 3.024 2274421479450009088 307.37182169671 +70.39970246304 11.8381 11.3149 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 131799_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131799_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:06.43 +69:58:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 4.051 2250388560449246592 306.52928903598 +69.97529650264 11.8894 11.5273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131800_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131800_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 131801_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131801_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:29.34 +73:27:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.975 2276134376829993600 306.37160349099 +73.45276675474 11.9571 11.4221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131802_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131802_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:47.08 +69:58:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.452 2250388732247828352 306.69587294162 +69.96752943304 11.8602 11.2771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131803_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131803_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 131805_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131805_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131806_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131806_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131808_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131808_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 131809_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131809_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131810_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131810_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 131812_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131812_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:52.99 +73:42:56.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
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Considering the candidate 131813_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131813_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:32:29.76 +68:02:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.214 2247077823560865920 308.12421134464 +68.04230011737 11.7602 11.2850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131814_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131814_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131817_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131817_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 131819_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131819_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131820_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131820_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:22.21 +70:22:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.942 2274603276825458048 306.84462907603 +70.37738524878 11.6536 11.1803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131821_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131821_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131822_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131822_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:17:59.04 +67:55:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.035 2249723901372408448 304.49529059826 +67.91860592316 11.3177 10.8801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131823_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131823_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131825_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131825_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:14:35.76 +70:44:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 5.853 2251418867265968256 303.65391517405 +70.74815643421 11.3948 10.9347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131826_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131826_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:04.58 +66:28:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.059 2246407911741882496 307.26757761741 +66.47726034133 11.3346 10.8295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131827_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131827_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:50:54.96 +65:07:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.109 2197577711298131840 312.73035021524 +65.12956022171 11.5190 11.0777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131830_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131830_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:42:44.70 +66:01:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.309 2245909046998566272 310.68710597829 +66.02837851060 11.6528 11.2995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131832_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131832_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:52:28.26 +68:46:11.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)
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Considering the candidate 131833_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131833_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:21.60 +67:53:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 1.713 2247096309100119424 307.34094224504 +67.89320601735 11.5641 11.1067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131834_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131834_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131835_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131835_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 131836_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131836_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:00.05 +69:07:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.794 2250279223463879808 306.99968874368 +69.12456439833 11.5439 11.0888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131838_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131838_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131839_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131839_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:58.70 +66:37:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 5.280 2246411455092745216 307.24125443271 +66.62944505310 11.3735 10.8991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131841_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131841_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:14:39.87 +70:52:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.497 2251433165214378752 303.67076043815 +70.88305842089 11.3041 10.8032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131842_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131842_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131843_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131843_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131845_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131845_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131846_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131846_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131848_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131848_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:37.03 +65:56:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 5.729 2245590222986652416 309.15775457716 +65.95026296604 11.4207 10.9388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131849_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131849_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:48.42 +66:27:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 2.124 2246358884693225728 309.20217491573 +66.45026822839 11.4059 10.9878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131850_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131850_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:33.65 +71:27:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.841 2274734908983368832 306.14178927734 +71.46578972855 11.6348 11.0730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131851_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131851_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:15.70 +73:26:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.249 2287979900929258112 301.56143555781 +73.43976913304 11.3845 10.8352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131852_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131852_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:05.61 +65:37:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 4.136 2245520403995796480 310.02108458021 +65.62790331861 11.2838 10.8850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131854_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131854_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131856_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131856_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:15:45.43 +72:08:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.565 2275577444128582784 303.94153505348 +72.14278681681 11.4579 10.9433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131857_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131857_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:13.16 +71:33:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.558 2274817746016300672 307.05747902390 +71.55500207303 11.8144 11.4121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131858_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131858_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:20:57.08 +68:50:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.889 2250198894693809280 305.23816901360 +68.85046246720 11.5361 11.0512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131859_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131859_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 131860_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131860_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131861_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131861_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131864_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131864_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:15:25.93 +70:07:50.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)
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Considering the candidate 131865_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131865_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131866_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131866_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:19:00.71 +72:10:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.750 2275656845187328768 304.75055435632 +72.16912586980 11.4526 11.0082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131867_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131867_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 131868_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131868_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131869_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131869_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:01.24 +67:46:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.742 2247088994774035840 307.00716552788 +67.76818830346 11.4033 10.9646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131870_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131870_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 131871_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131871_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131872_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131872_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 131873_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131873_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131874_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131874_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:28:07.59 +71:28:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.790 2229744950461874688 337.03206167498 +71.47797573102 12.8238 12.1985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131875_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131875_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:07.69 +73:49:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.360 2276342876018910720 305.28103679537 +73.82488540859 11.4272 10.8592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131876_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131876_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:30:14.04 +66:32:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 3.331 2246398089154556672 307.55811365125 +66.54474578968 11.1352 10.6910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131877_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131877_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:46:32.48 +65:50:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 3.072 2245705946585409792 311.63526140770 +65.83982491658 11.3947 10.9807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131878_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131878_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:34.79 +65:34:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 5.755 2245546895356337408 309.14263630586 +65.56905564903 11.1672 10.6789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131880_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131880_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:21.35 +68:34:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 4.173 2250190648356337408 305.33661708122 +68.57205091361 11.1331 10.8433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131881_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131881_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:03.31 +69:51:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.286 2250546237287823232 305.76472375115 +69.86023180780 11.5449 11.0679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131882_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131882_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:26.72 +68:48:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.293 2250218754622657152 305.86103593893 +68.80361929945 11.3014 10.8180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131884_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131884_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:47:27.47 +65:54:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 4.937 2245707110518749184 311.86744445353 +65.90262775638 11.5276 10.9875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131885_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131885_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 131886_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131886_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:13:56.90 +69:30:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.958 2250478922263201152 303.48851772170 +69.51245888154 11.1152 10.6465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131887_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131887_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 131888_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131888_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:33:20.38 +69:59:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.526 2274349392719028224 308.33457266396 +69.98986429561 11.5233 10.9996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131891_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131891_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 131892_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131892_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:17:23.34 +70:57:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.939 2251425743510942208 304.35060080371 +70.95731958020 11.2961 10.9186 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 131893_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131893_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 131894_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131894_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 131895_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131895_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 131896_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131896_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:01:35.67 +66:04:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 3.163 2197733837650491776 315.39982402873 +66.07371267997 11.8716 11.0229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131897_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131897_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:13.54 +67:55:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 3.728 2247105414430784256 306.55897511611 +67.92569880290 10.9940 10.4971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131898_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131898_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131899_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131899_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 131900_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131900_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:07.61 +69:19:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.988 2250250915337852544 305.28105717839 +69.31930757962 11.1486 10.8737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131901_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131901_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:18:51.86 +66:22:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 2.265 2246532538810426112 304.71594407796 +66.37720677418 10.7913 10.3213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131902_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131902_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131906_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131906_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131907_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131907_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:16:00.17 +71:55:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 2.790 2275557137523062400 304.00295400453 +71.92016085948 11.1268 10.6680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131908_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131908_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:29.08 +70:27:52.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)
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Considering the candidate 131909_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131909_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:07.04 +70:41:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.923 2274630317939498240 306.28062723680 +70.69673655372 11.1512 10.6353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131910_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131910_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:27.50 +72:33:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.815 2275692824129951872 305.86522976497 +72.55438312451 11.1990 10.7399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131911_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131911_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 131912_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131912_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:16:34.52 +67:44:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 3.679 2249761976260149248 304.14151220054 +67.73821540026 10.7397 10.3802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131913_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131913_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:46:42.51 +65:35:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 4.304 2245685193303323264 311.67998137763 +65.59977512416 11.0101 10.7139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131914_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131914_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 131915_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131915_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:55.79 +69:09:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 3.527 2250276822579807616 306.73406997511 +69.15217776588 11.1054 10.6712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131916_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131916_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:15.29 +66:14:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.707 2246490310691993088 306.06132201539 +66.23632593339 10.5179 10.1318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131917_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131917_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131918_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131918_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131919_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131919_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:06.05 +69:24:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.065 2250336466788023680 306.27583966718 +69.41411004216 11.0272 10.6394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131920_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131920_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:17:41.16 +66:26:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.999 2246542674933239552 304.41925263782 +66.44181878834 10.2014 9.9175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131921_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131921_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:17:02.07 +67:35:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.802 2249713013630312832 304.25732122504 +67.58986484968 10.4579 10.0049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131922_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131922_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:01:35.47 +66:04:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 3.737 2197733841949188992 315.39667520578 +66.06798271119 11.7457 11.3852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131924_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131924_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:07.76 +67:08:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 2.816 2246682312910017152 305.28065265011 +67.14607009016 10.4077 9.9989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131925_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131925_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 131926_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131926_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 131927_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131927_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 131928_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131928_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131929_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131929_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:32:52.37 +65:39:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 5.429 2245466321771138304 308.22043031210 +65.66183703226 10.2672 9.7943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131930_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131930_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131931_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131931_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:48:28.33 +64:58:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 3.271 2245232881708332672 312.11590566073 +64.97332263083 10.4550 10.2248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131932_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131932_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:50.82 +66:07:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 3.086 2246288722108077440 307.20976303221 +66.12012961717 10.2244 9.9488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131934_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131934_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:44:46.51 +65:34:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 5.451 2245696463297426688 311.19016862954 +65.58133359226 10.5817 10.2214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131935_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131935_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:03.17 +65:22:42.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)
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Considering the candidate 131937_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131937_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:32.14 +69:24:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 4.606 2250330801728696192 306.13033638363 +69.40130328416 10.4530 10.1035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131939_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131939_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:17.92 +66:16:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 1.818 2246306142495463808 306.82357561660 +66.27686141115 9.9985 9.6604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131940_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131940_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131941_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131941_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 131942_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131942_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:50.66 +67:06:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.33, MAG_FAINT_SEARCH_LIMIT=12.31)GAIADR2_OUTPUT=# 4.203 2246673345018374144 305.95848509107 +67.10088855310 9.8155 9.5131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131943_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131943_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 131944_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131944_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131946_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131946_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 131947_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131947_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131948_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131948_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:14:49.29 +67:45:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 2.316 2249764553240501632 303.70470222612 +67.76692424685 9.4622 9.1790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131949_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131949_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131950_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131950_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:38.78 +67:09:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 3.321 2246683103184013568 305.41080039866 +67.14915675200 9.5475 9.1635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131951_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131951_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:20:09.77 +67:25:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 5.390 2249697929707950720 305.03701753545 +67.43256994985 9.4935 9.2229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131952_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131952_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131953_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131953_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 131954_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131954_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:54.72 +73:32:10.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 131955_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 131955_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 131956_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131956_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 131957_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131957_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:36.82 +67:00:25.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131958_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131958_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 131959_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131959_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 131960_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131960_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:15:16.25 +72:08:07.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131961_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131961_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:18.84 +73:13:49.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131962_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131962_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 131963_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131963_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:19:22.29 +64:52:23.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 131971_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131971_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:25.35 +73:54:36.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131973_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131973_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:13:19.75 +72:53:50.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131976_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131976_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:12.40 +69:30:43.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131977_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131977_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:18:08.01 +70:47:07.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131981_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131981_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:52.37 +72:46:59.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131987_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131987_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:56:43.56 +72:18:38.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131988_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131988_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:13:15.93 +71:06:27.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131995_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 131995_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:20.40 +73:09:07.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132006_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132006_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:27.41 +70:39:33.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132012_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132012_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:49:55.27 +64:59:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.38, MAG_FAINT_SEARCH_LIMIT=10.36)GAIADR2_OUTPUT=# 2.792 2197569430597680512 312.47850490835 +64.98684155439 8.3664 7.4376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132013_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132013_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:11:38.90 +73:58:48.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132017_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132017_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:41:22.54 +65:02:20.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132020_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132020_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:11:26.14 +71:59:11.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132021_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132021_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:47.10 +72:59:51.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132024_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132024_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:17:02.62 +72:52:48.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132026_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132026_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:10:03.57 +70:50:17.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132028_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132028_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:56:39.72 +72:56:18.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132054_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132054_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 132073_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132073_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:46.06 +65:25:39.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132074_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132074_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:12.18 +65:51:16.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132077_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132077_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132079_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132079_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:25.20 +70:03:40.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132081_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132081_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:36.34 +72:22:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.41, MAG_FAINT_SEARCH_LIMIT=11.39)GAIADR2_OUTPUT=# 2.042 2275810025197169664 301.14963378632 +72.38026953467 9.1334 8.6437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132088_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132088_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:56:27.10 +73:36:57.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132089_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132089_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:27.49 +65:33:54.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 132091_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132091_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:01:17.03 +72:54:15.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132092_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132092_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:26.68 +73:13:54.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132094_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132094_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:03.92 +72:56:18.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132095_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132095_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 132110_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132110_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132118_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132118_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:06.52 +65:16:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.48, MAG_FAINT_SEARCH_LIMIT=11.46)GAIADR2_OUTPUT=# 3.951 2245477248166645376 310.02542269135 +65.27187465220 9.4023 8.0955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132136_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132136_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:30:34.27 +65:27:07.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132154_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132154_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:57:29.06 +72:19:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 4.984 2263811089162557440 299.37561995089 +72.33163255009 9.4045 9.1107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132164_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132164_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132169_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132169_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:46:24.82 +65:03:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 2.794 2245248240511367168 311.60303304315 +65.05362994750 9.8251 8.7371 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132178_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132178_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:38:22.62 +64:57:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 0.892 2245373103800750976 309.59368373845 +64.96613180754 9.7012 8.8223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132195_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132195_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 132196_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132196_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132197_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132197_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:03:01.12 +72:37:11.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132200_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132200_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:23.31 +64:58:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 2.735 2245382582790254336 308.84533044180 +64.97230910633 9.6352 8.8605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132210_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132210_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:18.67 +65:32:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 1.861 2246246871946229120 306.07888972584 +65.54096836555 9.4274 8.6044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132216_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132216_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:30:41.54 +65:44:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 3.902 2246220552386986752 307.67054337367 +65.73787393301 9.4644 9.0141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132231_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132231_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:08:39.92 +73:06:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 4.460 2275956741279254016 302.17043101778 +73.11509426537 9.8299 9.4649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132238_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132238_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132241_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132241_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:20:36.30 +66:09:00.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132243_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132243_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132251_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132251_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:40.18 +64:47:43.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132255_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132255_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 132272_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132272_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:07:25.49 +64:57:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 1.629 2197390278925170176 316.85638002513 +64.95050207984 10.5973 9.8062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132273_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132273_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132285_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132285_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132286_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132286_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132292_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132292_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:57:52.44 +72:11:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 5.819 2263800403283937280 299.47365417515 +72.19727655459 9.8329 9.4764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132299_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132299_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132308_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132308_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:57:26.14 +67:09:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 1.350 2219652537530210304 329.35938184490 +67.15636579730 10.7001 9.2597 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132310_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132310_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132312_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132312_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:54:14.98 +73:23:22.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132314_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132314_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132315_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132315_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132334_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132334_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:32.93 +65:04:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 0.586 2245392001656834560 308.88744607541 +65.06968387244 10.2079 9.4258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132339_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132339_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 132343_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132343_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:08:33.73 +73:12:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.807 2275963922464568064 302.14469192689 +73.21394976836 10.1417 9.7579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132347_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132347_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132353_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132353_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:59:30.51 +72:14:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 2.147 2251797172283829632 299.87869728713 +72.23368745956 10.1592 9.7047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132358_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132358_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 132360_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132360_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:31.14 +64:51:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 4.677 2244666976817560320 306.88220954759 +64.86263331655 9.9104 9.3124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132365_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132365_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132373_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132373_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:24.71 +65:03:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 1.251 2245468830030591616 309.85232343945 +65.05113791937 10.3492 9.5278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132377_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132377_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:58:23.10 +71:49:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 4.031 2251759410931085696 299.59276721821 +71.82054787658 10.0729 9.3283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132381_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132381_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132383_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132383_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:33.76 +64:55:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.538 2245276449856159744 310.13999468080 +64.92870929154 10.3496 9.3524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132384_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132384_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:02:40.12 +71:04:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 3.996 2251664646772609408 300.66374838073 +71.06951933014 10.2056 9.7231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132388_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132388_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132393_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132393_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:58:18.98 +72:13:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 0.872 2263800884318684800 299.57980948368 +72.22287536693 10.1875 9.7168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132406_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132406_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132416_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132416_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:31:44.95 +65:03:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 1.103 2245413167255482752 307.93798577555 +65.05764647603 10.2574 9.4564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132422_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132422_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:12:27.58 +73:19:23.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 132426_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132426_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132429_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132429_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:22.78 +71:45:44.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132431_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132431_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:03:44.86 +71:36:25.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 132437_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132437_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 132467_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132467_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 132473_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132473_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132478_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132478_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132487_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132487_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 132488_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132488_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 132506_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132506_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132508_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132508_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 132516_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132516_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:17.31 +65:31:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 5.513 2246202582243528704 306.56889369412 +65.51847903891 9.8767 9.5390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132520_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132520_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132524_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132524_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 132527_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132527_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132528_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132528_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 132530_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132530_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132537_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132537_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:37:22.78 +65:09:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 2.285 2245484257550025088 309.34574857668 +65.16672448538 10.6373 9.7975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132551_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132551_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:57:03.04 +73:33:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 0.682 2287949247745628928 299.26200438296 +73.55486049183 10.4268 9.7199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132552_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132552_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:12:31.67 +64:55:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.319 2220646736559296384 318.13258724472 +64.92097361874 11.3594 10.9532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132557_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132557_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 132558_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132558_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:58:59.78 +72:01:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 1.685 2251787379758289792 299.75055325076 +72.01819798991 10.4380 9.9807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132566_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132566_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:32:42.51 +64:53:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 0.605 2245407600977821312 308.17704285310 +64.89783554790 10.4481 9.6327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132578_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132578_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132579_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132579_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132583_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132583_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 132587_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132587_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:13:19.27 +74:04:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 1.297 2276391014012238080 303.33087016306 +74.07471238761 10.7997 10.4114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132588_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132588_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (34.3") between the two second-epoch detections
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Considering the candidate 132589_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132589_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132590_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132590_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132591_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132591_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 132592_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132592_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:46:32.66 +65:00:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 1.222 2245247106639939328 311.63660154210 +65.00529629284 10.9133 9.9844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132593_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132593_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:59.43 +65:14:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.350 2245477110727613184 309.99674616730 +65.24793370257 10.4604 10.1488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132595_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132595_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132604_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132604_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 132605_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132605_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132622_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132622_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 132625_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132625_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132628_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132628_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:18.59 +64:57:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 4.928 2244677937574090752 306.32993030492 +64.95374354097 10.2569 9.6760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132634_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132634_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:09.96 +64:55:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 1.669 2244677112940313472 306.04189929750 +64.92195952308 10.2412 9.4443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132639_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132639_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:20:19.96 +65:34:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 4.636 2244948761028685952 305.08627921581 +65.57326279289 10.3978 9.5695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132660_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132660_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:32:59.12 +64:56:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 3.276 2245408150733636096 308.24809124895 +64.94902346237 10.5776 10.0743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132662_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132662_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132664_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132664_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:42:47.33 +65:12:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 2.732 2245308541852110720 310.69778103563 +65.20380311197 10.5932 10.1871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132671_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132671_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:23.07 +65:24:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 3.620 2244755040824892544 305.59850198007 +65.41509807606 10.5140 9.6514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132688_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132688_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132699_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132699_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:31.16 +65:07:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 1.772 2244687352140121984 306.38073612294 +65.11974242107 10.5554 9.6412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132719_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132719_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 132723_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132723_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 132731_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132731_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 132740_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132740_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 132743_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132743_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:49:00.92 +65:01:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 1.419 2245608571086556672 312.25451727109 +65.03078708612 11.1073 10.2125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132757_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132757_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:30:25.36 +65:39:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 3.379 2246219796470492032 307.60351570275 +65.65691939778 10.3744 9.9790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132761_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132761_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:55.84 +65:41:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.472 2246261371755953920 305.98234158566 +65.69416903495 10.7596 9.7077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132768_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132768_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:33:19.27 +64:55:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.661 2245407837197947776 308.32940247684 +64.92244127674 10.6760 10.0641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132771_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132771_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:25:25.30 +70:27:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.358 2272190810877028096 321.35798481063 +70.45174804310 12.1057 10.9168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132776_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132776_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 132787_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132787_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 132794_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132794_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132795_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132795_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:15:45.87 +68:57:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 5.737 2250400375901277056 303.94399634905 +68.96335441992 10.7576 10.3770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132797_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132797_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132800_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132800_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132809_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132809_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132812_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132812_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 132814_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132814_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132816_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132816_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 132820_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132820_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 132832_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132832_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:22.15 +65:05:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.305 2245390760407980544 309.09149628909 +65.09033407986 10.6983 10.2082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132839_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132839_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:00.00 +65:12:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 4.969 2246188494750669184 306.75294059460 +65.20214760598 10.6531 10.1017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132844_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132844_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 132846_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132846_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:50.10 +65:18:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 3.118 2244748375037868416 305.46070469207 +65.31209480881 10.7006 9.8799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132867_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132867_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132877_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132877_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132880_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132880_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 132887_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132887_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132890_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132890_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:43:12.56 +64:58:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.856 2245268066080201600 310.80277996422 +64.97156103254 11.1325 10.3102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132891_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132891_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:44.27 +65:37:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 2.418 2246259275809052544 305.93599094172 +65.63042055794 10.6576 10.1319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132892_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132892_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 132896_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132896_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132904_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132904_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132909_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132909_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 132912_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132912_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:00:25.59 +71:34:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.355 2251739791520512000 300.10461714213 +71.57646030724 10.9574 10.5878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132919_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132919_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132925_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132925_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 132928_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132928_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:01:00.21 +72:49:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 2.567 2287844592279541632 300.25218395297 +72.82109916492 11.1257 10.6937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132940_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132940_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:58:43.36 +71:54:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 3.863 2251760166845502848 299.67721429197 +71.90628804754 10.8549 10.0819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132943_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132943_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 132944_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132944_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:55:17.09 +70:16:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 4.025 2225859486827616896 343.82445107726 +70.27450608742 12.1358 10.9472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132949_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132949_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 132952_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132952_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 132960_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132960_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:35.95 +65:23:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.024 2244754765949286912 305.65047465309 +65.39346535265 10.9134 10.0121 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 132964_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132964_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 132984_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 132984_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 132989_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132989_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:22.92 +65:02:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.440 2245388119006405376 309.09621727840 +65.03413421178 11.1967 10.4464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132997_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 132997_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:59:34.35 +71:40:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.197 2251744395725438464 299.89149708303 +71.67888796748 11.0015 10.2301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133004_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133004_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133011_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133011_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:16.91 +71:29:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.781 2251700930656505728 301.57258498393 +71.48993073814 11.2810 10.7991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133015_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133015_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:57.23 +65:40:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 4.803 2246226462261887744 307.23587993686 +65.67208139884 11.2181 9.9824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133030_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133030_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 133045_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133045_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 133060_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133060_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 133062_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133062_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 133066_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133066_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 133067_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133067_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:45:47.91 +65:11:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.694 2245253153954006912 311.44987213486 +65.18525409447 11.4336 10.5980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133083_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133083_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 133086_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133086_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133088_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133088_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 133093_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133093_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 133103_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133103_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:20:20.16 +66:01:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 3.945 2246471928231786496 305.08185055988 +66.03197668621 10.5438 10.1961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133107_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133107_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:02:25.79 +71:16:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.797 2251680108654867328 300.60954604856 +71.27358742077 11.2090 10.7565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133110_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133110_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 133112_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133112_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:02.16 +65:11:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.351 2246177156037035008 307.00984424733 +65.19609609962 11.0890 10.2049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133114_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133114_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133119_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133119_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 133122_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133122_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133125_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133125_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:11:33.30 +73:12:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.285 2275952377592510208 302.88868796684 +73.20555086967 11.4187 10.9076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133132_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133132_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 133133_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133133_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 133134_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133134_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 133135_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133135_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:48.80 +65:03:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.916 2246172551832058880 307.20161268385 +65.05894347218 11.2247 10.3152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133138_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133138_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:46.59 +72:10:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.525 2275757076840004864 301.69384511285 +72.17361795664 11.2314 10.7141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133145_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133145_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:42:28.59 +65:41:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 3.179 2212440909482808576 340.62072773473 +65.68921869330 12.3133 11.1616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133150_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133150_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:42:43.43 +65:19:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 0.525 2217902630415876992 325.68112427631 +65.32090595722 12.5419 11.1082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133173_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133173_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:45.12 +64:47:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 3.802 2244654813469926912 305.68646860904 +64.79869703033 10.9519 9.8365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133174_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133174_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:12:03.90 +71:24:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 3.570 2251500402926196736 303.01935701690 +71.40993653223 11.1893 10.5968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133189_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133189_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 133205_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133205_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:34:13.02 +64:55:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.365 2245383480441548800 308.55340929132 +64.92418488559 11.3666 10.2893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133217_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133217_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 133218_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133218_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133220_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133220_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133233_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133233_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:07:31.27 +73:14:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.727 2275961272468351744 301.88121671571 +73.23326335697 11.6512 11.3813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133237_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133237_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133244_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133244_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:38:40.73 +65:16:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 2.471 2245475010485445632 309.66808748890 +65.26689306278 11.4937 10.5341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133248_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133248_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:58.54 +73:21:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 3.675 2287978698338427520 301.74542012078 +73.36437983234 11.3383 10.8526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133272_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133272_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 133280_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133280_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:32:12.85 +64:57:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 3.294 2245411655426944256 308.05390328922 +64.96006885338 11.4047 10.6062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133286_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133286_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:31:18.07 +65:13:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.938 2245450481931457536 307.82500538900 +65.22489793637 11.3478 10.4401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133290_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133290_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 133297_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133297_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 133300_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133300_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 133305_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133305_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:39.61 +65:10:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.089 2245391520620601984 309.16463607212 +65.17897297574 11.6092 10.6647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133318_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133318_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:12.19 +65:08:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 0.548 2244688898330772480 306.30067804018 +65.13670007005 11.3364 10.3799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133320_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133320_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 133327_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133327_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:47:29.67 +65:27:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 4.196 2245680108061978240 311.87097253649 +65.46181333392 11.7683 10.8782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133342_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133342_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133366_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133366_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:57:34.50 +66:07:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.319 2219267330505684096 329.39641896698 +66.12167262412 12.9484 12.3913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133370_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133370_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133389_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133389_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:41:10.28 +65:06:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.140 2245286998296024576 310.29358002928 +65.11445625691 11.6461 10.8187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133407_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133407_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:09.50 +64:51:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.873 2245369014991765888 309.04080579320 +64.86600664419 11.6210 11.0354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133408_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133408_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133409_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133409_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:05:09.21 +71:21:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.766 2224478156623123712 331.29018330893 +71.35995058138 12.1042 10.4617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133415_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133415_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133416_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133416_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133422_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133422_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 133434_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133434_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:09:54.54 +71:12:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 3.279 2251502984201265664 302.47969347154 +71.20884751657 11.4190 11.1078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133457_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133457_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:00:58.62 +73:31:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.354 2287993095068734848 300.24827997575 +73.52982536560 11.5919 11.1610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133464_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133464_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 133466_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133466_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:03:08.06 +72:25:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.901 2275816416108293760 300.78614766111 +72.42372253638 11.4740 11.0688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133471_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133471_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133475_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133475_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:29:06.33 +69:25:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.142 2226233045903134848 337.27400111789 +69.43014551981 13.2890 12.6985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133483_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133483_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 133495_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133495_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:03.75 +65:00:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.441 2245385885623348224 308.76513696056 +65.01170544791 11.4673 10.5499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133500_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133500_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 133507_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133507_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:38:45.92 +65:02:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.598 2245467146403409280 309.69044069966 +65.03734583554 11.7842 11.2388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133516_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133516_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:21.19 +65:55:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 5.511 2246284770738075008 307.09183108773 +65.92526871700 11.1689 10.7670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133517_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133517_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:40.72 +64:50:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.420 2244675635471504640 306.17032502880 +64.84500009950 11.2684 10.4637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133526_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133526_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:04.47 +65:30:13.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)
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Considering the candidate 133529_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133529_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:01:17.66 +71:49:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 4.846 2251769650133338752 300.32265063431 +71.81940803284 11.2680 10.7959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133552_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133552_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133561_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133561_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133562_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133562_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:09:39.32 +72:36:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 4.250 2275792914047334016 302.41749391442 +72.61486088697 11.7681 11.2942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133567_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133567_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 133580_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133580_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:52:34.24 +67:58:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.588 2213323782961042048 343.14370035397 +67.97034545165 12.9279 12.2434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133585_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133585_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 133586_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133586_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:00:26.23 +71:25:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.838 2251732060579632000 300.11347316795 +71.42007494787 11.3785 10.9736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133587_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133587_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:52.38 +71:06:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.844 2251479684003577088 301.71685807735 +71.10381224895 11.4088 10.8075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133590_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133590_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133594_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133594_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:03:44.87 +73:15:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.968 2287974059773614336 300.94068205447 +73.26416094655 11.4976 10.9958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133605_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133605_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:43:13.00 +65:19:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.691 2211668326467997184 340.80517484998 +65.31673631959 12.9083 12.3065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133606_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133606_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:26:52.50 +65:28:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 0.899 2206652771037211392 336.71815207426 +65.47322201884 12.9767 12.1933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133615_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133615_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:08:56.60 +71:21:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.225 2251508202586808192 302.24025843748 +71.36481149938 11.6278 11.1075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133618_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133618_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:54.27 +65:29:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.978 2246210553702939136 307.47515288824 +65.49113870300 11.7117 10.6870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133619_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133619_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 133633_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133633_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133634_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133634_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:00:59.28 +72:58:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.358 2287869984126381056 300.24875451844 +72.97903809118 11.5919 11.1223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133639_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133639_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133645_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133645_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 133649_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133649_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:58:44.99 +72:45:56.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 133651_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133651_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:59:43.66 +72:49:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 0.949 2287843694630097664 299.93269553710 +72.82059368593 11.8002 11.2920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133654_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133654_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:39.66 +65:15:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 5.726 2245477656185300608 310.16830848014 +65.25311028292 11.6337 11.1444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133677_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133677_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 133697_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133697_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133702_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133702_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:30:56.33 +65:15:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.843 2245453711746915072 307.73418025276 +65.26374419113 11.6580 10.9826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133706_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133706_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 133714_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133714_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:07:11.61 +72:46:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.722 2275845651948379392 301.79862308102 +72.77768661654 11.7593 11.2626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133716_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133716_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:32:42.71 +64:55:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 5.191 2245407635337558784 308.17888548008 +64.92013727776 11.4027 10.8067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133718_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133718_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133723_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133723_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:57:51.45 +73:13:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.870 2287934958391576064 299.46259601648 +73.23160700173 11.6302 11.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133735_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133735_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 133740_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133740_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 133746_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133746_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133748_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133748_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 133755_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133755_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:23.96 +65:01:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.446 2244728927425759616 305.60196546775 +65.02171397623 11.3973 10.6096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133763_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133763_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:08.03 +72:34:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.242 2275836035518941312 301.53448889347 +72.57726561141 11.6529 11.1977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133785_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133785_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:03:34.11 +72:19:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.043 2275804149681536384 300.89673883673 +72.33315124716 11.9082 11.4397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133786_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133786_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:23.08 +65:17:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.509 2244741503090243456 305.84704664016 +65.28924369418 11.4377 10.4712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133795_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133795_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:38:07.88 +65:19:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.406 2245487281210158464 309.52990720840 +65.32436908909 11.7495 11.2155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133798_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133798_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 133799_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133799_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133807_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133807_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:07:29.59 +72:35:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.125 2275834489330731136 301.87597138157 +72.58672130930 11.7173 11.2865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133813_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133813_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 133818_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133818_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:32:18.74 +72:52:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.172 2230998775973102336 338.08199121898 +72.87091510044 13.5106 12.8995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133824_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133824_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:10.87 +65:17:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.106 2245442957148959488 308.79401537761 +65.29999070617 11.5615 10.9698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133835_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133835_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:10:27.77 +71:16:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 5.719 2251503671397607552 302.62061848782 +71.27732946031 11.9020 11.4115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133840_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133840_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:32:43.65 +73:11:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 4.573 2231056981370071296 338.18504366962 +73.18601845745 13.3648 12.6740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133841_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133841_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:22.69 +64:52:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.829 2245368602674906880 309.09139007505 +64.87027112833 11.8313 10.9354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133852_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133852_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:51:24.48 +71:47:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.972 2226990815572771328 342.85032725903 +71.79475261545 13.5732 13.0212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133857_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133857_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 133866_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133866_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:30.73 +65:04:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.828 2245468967469561472 309.87910671516 +65.07501509731 11.7998 10.8773 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 133871_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133871_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 19:56:07.71 +72:43:13.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 133877_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133877_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 133901_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 133901_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 133917_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133917_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:57.53 +65:10:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.755 2246176331403287296 306.74264663498 +65.17480507917 11.4797 10.9134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133927_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133927_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:14:56.26 +72:24:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.215 2275865924195245056 303.73644592538 +72.40073085151 12.0065 11.4863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133929_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133929_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:28.68 +64:49:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.720 2244665087031830272 306.37124932532 +64.81868528532 11.4407 10.8050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133930_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133930_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:25:21.30 +70:27:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.583 2272190810877027328 321.33922070411 +70.45016123590 13.5666 12.6184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133936_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133936_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:57:51.13 +68:25:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.302 2213360238643850368 344.46687701073 +68.42284040037 13.0625 11.9860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133942_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133942_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:24.06 +65:04:13.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 133953_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133953_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 133960_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133960_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:16.17 +70:53:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.977 2251467696751279744 301.56510802889 +70.88346902406 11.7704 11.2195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133963_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133963_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:05:15.81 +71:35:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.681 2251714159155758592 301.31792220421 +71.59254111482 11.5588 10.9925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133973_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 133973_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:53.93 +73:50:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.695 2288024289414316416 301.22529799027 +73.84990208280 12.0010 11.4866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134013_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134013_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:32:16.05 +72:50:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.601 2230997573382267520 338.07033772492 +72.83448265856 13.2696 12.3119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134023_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134023_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:45:08.79 +65:08:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.730 2245293698445216768 311.28689529278 +65.13838898358 12.1640 11.2480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134029_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134029_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134056_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134056_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:25:59.21 +65:27:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.055 2246196500569793152 306.49514736741 +65.46113441489 11.8232 10.9187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134072_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134072_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:57.15 +64:57:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.798 2245278305282026880 309.98809688358 +64.96175096642 11.9858 11.5328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134083_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134083_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134093_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134093_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 134098_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134098_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134099_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134099_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134116_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134116_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:08.78 +64:55:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.158 2245369800967584256 309.03597832190 +64.92349969650 12.2194 10.9675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134117_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134117_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:23.14 +65:10:19.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 134119_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134119_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:21.53 +71:50:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.738 2251726391222820864 301.08805056268 +71.84519695413 11.8216 11.2609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134123_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134123_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 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 134133_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134133_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:42:20.02 +65:00:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.675 2245272086169582336 310.58236978576 +65.00877447698 11.9708 11.1236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134137_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134137_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 134139_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134139_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:14.34 +71:41:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.002 2251718660281464704 301.06017418372 +71.69314466558 11.6637 11.1260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134147_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134147_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:33:50.61 +64:50:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.842 2245359699204495104 308.45973423454 +64.84671028237 11.8328 10.9848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134162_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134162_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:32.79 +64:52:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.977 2245380937820919552 308.88415009236 +64.88261950306 12.0896 11.1650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134165_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134165_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:23:18.90 +67:09:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.631 2219063371096315264 335.83060742871 +67.15274348284 13.1554 12.1584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134182_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134182_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134186_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134186_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:50:39.81 +65:05:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.759 2197571659685167616 312.66344899012 +65.08543640562 12.2285 11.3621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134188_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134188_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:28:04.54 +64:55:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 4.554 2244669072761702144 307.01766209196 +64.93104663788 11.7514 10.8310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134198_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134198_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:43:03.00 +65:00:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.371 2245271467694297344 310.76403309570 +65.00260292550 12.0281 11.2478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134201_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134201_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:35.30 +65:11:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.241 2244734768581436416 305.64637696988 +65.19076850605 11.7430 10.9358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134208_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134208_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:37.91 +65:12:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.543 2246178045093372288 306.90697125778 +65.20916253329 11.8497 11.0057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134213_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134213_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134224_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134224_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 134253_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134253_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134259_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134259_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134283_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134283_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:42:12.15 +65:09:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.347 2245285142870280320 310.55273858146 +65.16630465814 12.0370 11.4964 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134310_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134310_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134323_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134323_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134349_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134349_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:04:14.25 +73:47:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.820 2288026664533144320 301.05952579734 +73.79966841088 11.8478 11.3656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134359_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134359_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:48.64 +65:16:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 4.017 2246188975787027840 306.70524934699 +65.26700021781 11.8411 11.2599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134363_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134363_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:33:07.37 +65:13:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.352 2245439315016549376 308.27920654616 +65.22451934446 11.9330 10.9605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134392_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134392_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:50.64 +64:46:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.316 2244660585906174208 306.70926420929 +64.78130651175 11.8883 10.8943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134393_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134393_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:21:52.11 +65:49:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.397 2246453580131449600 305.46653312733 +65.82438000200 11.8237 10.8236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134405_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134405_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134438_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134438_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:03:21.53 +73:53:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 5.798 2288028446942656896 300.83425883031 +73.89805607713 11.6014 10.7823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134468_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134468_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:06:10.46 +73:04:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.425 2275958592409616768 301.54371588114 +73.07522263850 12.0463 11.5504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134469_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134469_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134514_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134514_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 134522_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134522_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 134566_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134566_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:53:03.12 +65:03:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.037 2197562421214570496 313.26219308026 +65.05358919413 12.5413 11.6894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134588_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134588_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:59.40 +65:09:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.486 2244736658367054208 305.99653321250 +65.16285236991 11.7421 10.8372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134596_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134596_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:03.69 +65:01:15.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)
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Considering the candidate 134599_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134599_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:45:55.96 +64:58:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.803 2245241471642780160 311.48404366585 +64.96912887538 12.4110 11.9187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134611_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134611_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:58:19.34 +65:01:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 4.640 2197526893245390208 314.57822430362 +65.01848771327 12.7040 11.7977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134612_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134612_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:35:35.60 +64:57:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.664 2245381762454695296 308.89684355541 +64.95211849900 12.1557 11.1639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134614_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134614_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:19.30 +64:57:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.229 2245276789155550976 310.07961233190 +64.96427517823 12.1425 11.5482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134649_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134649_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 134659_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134659_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134672_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134672_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:43:20.74 +65:01:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.349 2245268650195752448 310.83715245481 +65.01890378212 12.0557 11.5831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134677_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134677_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:39.19 +64:52:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.671 2245415503717463168 307.41235935259 +64.87543677100 11.7547 11.1742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134703_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134703_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:52:23.22 +65:00:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.196 2197572449959980672 313.09479038981 +65.01573477559 12.7667 11.9613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134704_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 134704_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 134725_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134725_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 134736_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134736_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:50:31.79 +65:03:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.338 2197571041209877376 312.63175587418 +65.05530316558 12.5923 11.7450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134753_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134753_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:48:43.11 +64:58:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.204 2245233083568343552 312.17960203921 +64.98197111194 12.4652 11.5138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134759_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134759_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:26:42.09 +65:17:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.556 2246189731701270656 306.67685905949 +65.28357170943 11.9227 11.4031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134769_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134769_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:53:18.21 +71:36:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 3.013 2224727878905300864 328.32849183933 +71.61308316848 13.0645 11.4633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134774_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134774_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:48:19.76 +65:07:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.107 2245612969133076224 312.08124363515 +65.12444736798 12.5659 11.7696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134787_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134787_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:49.98 +65:44:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 4.872 2246232165978550912 307.45556718369 +65.73554832397 12.2055 11.4715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134799_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134799_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:59.73 +65:09:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.855 2245287273173995648 310.24764905532 +65.15542884504 12.5476 11.7052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134804_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134804_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:04.66 +65:02:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 2.929 2244682851016725888 306.01936349088 +65.03501991833 12.0233 11.1158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134809_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134809_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 134827_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134827_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 23:02:08.32 +72:10:34.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
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Considering the candidate 134837_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134837_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:50:19.81 +68:12:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.028 2222958253598631040 327.58391967267 +68.20212572534 12.8803 11.4071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134841_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134841_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:24:35.19 +65:14:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.689 2244738788670920192 306.14854027283 +65.24247355234 11.8920 11.0568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134857_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134857_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:17.56 +65:18:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.866 2245480267525414400 309.82140749605 +65.30308308745 12.2654 11.3658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134865_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134865_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 134875_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134875_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:13:31.92 +65:05:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.789 2218591263991602176 333.38407220570 +65.09135473262 12.6839 11.1609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134907_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134907_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:22:31.42 +65:18:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.696 2244742327721576832 305.62866940099 +65.31111217611 11.9660 11.1365 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 134931_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134931_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 134954_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134954_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:05.45 +64:49:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.845 2243913978853427456 307.27096597903 +64.81866251613 11.8522 11.0000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134965_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134965_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:43.82 +65:25:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.565 2245503395927584128 310.18113816658 +65.43278356149 12.9543 12.0003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134976_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134976_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:33:04.32 +64:51:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 4.595 2245360321977768576 308.26689636670 +64.84939613069 11.9604 11.3711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134977_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 134977_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:27:09.21 +65:52:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.697 2246279440680197504 306.78664756552 +65.87113842919 12.2043 11.3241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 135053_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 135053_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:33.77 +64:56:16.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)
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Considering the candidate 135061_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 135061_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:34:09.56 +65:01:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.908 2245385232788260608 308.53699582890 +65.02826589062 12.4825 11.7473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 135075_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 135075_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 135120_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 135120_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 135132_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 135132_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 135140_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 135140_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 135218_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 135218_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:03.58 +65:03:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.060 2245281363298867072 310.01338703456 +65.05204735217 12.6651 11.5120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 135282_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 135282_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:13:07.15 +65:32:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 4.534 2221441133710432128 318.27849842904 +65.53786001440 13.7022 12.3596 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 135306_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 135306_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:39:20.69 +64:58:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.718 2245279439153388288 309.83488175345 +64.97859337695 12.5998 11.7830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 135415_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 135415_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 135481_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 135481_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:40:35.76 +65:34:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.832 2245509580680576768 310.14737803515 +65.57517209999 12.8509 11.9116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 135503_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 135503_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 58561_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 58561_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:20:06.73 +68:52:53.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 15680_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 15680_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:03:11.21 +73:08:18.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 37629_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 37629_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 50876_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 50876_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 54330_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 54330_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 32251_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 32251_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 48528_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 48528_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 78533_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 78533_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 19496_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 19496_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 80207_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 80207_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 104236_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 104236_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 49473_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 49473_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 103278_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 103278_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 53016_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 53016_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 104873_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 104873_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 110311_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 110311_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:39:10.33 +68:16:13.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 108509_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 108509_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:20:01.81 +68:15:30.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)
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Considering the candidate 25748_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 25748_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 47606_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 47606_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:16:58.29 +70:15:44.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 108691_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 108691_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 38350_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 38350_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 97858_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 97858_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 98615_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 98615_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 81131_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 81131_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 84593_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 84593_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 51432_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 51432_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:40:10.00 +68:07:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.291 2225019322504801664 340.04315027274 +68.11940713256 12.1320 10.5331 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 48740_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 48740_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 24745_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 24745_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
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Considering the candidate 43260_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 43260_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 38214_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 38214_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 96832_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 96832_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 102552_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 102552_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 06638_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 06638_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 76001_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 76001_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:31:30.00 +67:23:49.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 73242_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 73242_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 66767_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 66767_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:59.93 +65:15:23.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 68171_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 68171_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 56969_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 56969_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 70442_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 70442_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 18333_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 18333_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 17267_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 17267_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 07458_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 07458_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:00:06.38 +74:35:21.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 94548_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 94548_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 70213_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 70213_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 86325_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 86325_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 72050_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 72050_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 84276_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 84276_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 93654_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 93654_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 34655_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 34655_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 106655_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 106655_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (25.2") between the two second-epoch detections
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Considering the candidate 31430_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 31430_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 88152_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 88152_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 51054_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 51054_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 74249_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 74249_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 40981_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 40981_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 39025_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 39025_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 15228_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 15228_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 18583_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 18583_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:20:33.78 +73:17:58.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 34117_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 34117_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:20:37.48 +71:31:11.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54716_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 54716_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 98536_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 98536_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 24609_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 24609_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 107474_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 107474_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 08775_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 08775_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 112093_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 112093_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:19:08.17 +68:41:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.140 2222479588081786496 319.78442931544 +68.69502741415 13.0923 12.5001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105686_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 105686_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 18504_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 18504_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 93684_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 93684_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 91547_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 91547_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:45:28.22 +66:00:19.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 59621_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 59621_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 61660_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 61660_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 49962_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 49962_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 98049_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 98049_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 105861_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 105861_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:46:12.18 +67:38:13.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 35268_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 35268_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 80790_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 80790_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 61030_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 61030_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 81078_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 81078_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:29:33.29 +67:02:14.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 47956_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 47956_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 106902_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 106902_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 20742_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 20742_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 108481_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 108481_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:36:38.90 +68:17:40.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 84175_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 84175_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 95296_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 95296_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72601_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 72601_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 19836_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 19836_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 57884_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 57884_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 30376_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 30376_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 70974_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 70974_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44186_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 44186_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95079_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 95079_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 92018_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 92018_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:28:05.98 +66:20:29.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 86948_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 86948_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 33383_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 33383_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 19447_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 19447_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:38:38.30 +73:03:04.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 102729_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 102729_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 73059_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 73059_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 109410_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 109410_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 76707_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 76707_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 70052_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 70052_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 28710_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 28710_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:49:13.36 +71:53:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.658 2272787703954580736 327.30704616621 +71.89643459116 12.5835 10.9971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54018_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 54018_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:23:50.76 +69:35:47.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 17879_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 17879_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 35503_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 35503_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 34057_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 34057_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 44266_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 44266_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:17:29.03 +70:30:50.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 29553_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 29553_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 67421_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 67421_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:32:02.74 +65:09:50.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51133_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 51133_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 37593_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 37593_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 45250_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 45250_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 61255_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 61255_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 31887_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 31887_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:57:34.37 +71:18:27.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 92918_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 92918_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 27602_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 27602_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 73482_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 73482_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 102594_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 102594_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 123860_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 123860_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:49:42.55 +72:15:48.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 59649_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 59649_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:23:25.13 +69:08:59.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 109534_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 109534_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 103760_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 103760_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 30145_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 30145_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:20:47.93 +71:59:54.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 21910_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 21910_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 42011_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 42011_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 53151_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 53151_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:26:55.65 +68:25:12.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 34606_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 34606_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 11655_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 11655_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 74496_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 74496_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:32:58.75 +66:54:44.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 61328_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 61328_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 96029_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 96029_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 84237_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 84237_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 38088_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 38088_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 44980_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 44980_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 26078_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 26078_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 23:00:10.25 +70:02:27.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 49525_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 49525_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 107518_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 107518_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:44:42.10 +67:49:30.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 87429_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 87429_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 43167_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 43167_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 103345_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 103345_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 74672_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 74672_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 12143_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 12143_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 80946_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 80946_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 72469_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 72469_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 25364_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 25364_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 102903_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 102903_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 67288_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 67288_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 21201_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 21201_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:47:49.84 +72:46:08.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 122828_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 122828_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:47:23.36 +71:19:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.394 2274896537192359680 311.84450488797 +71.32865136294 12.7068 11.2783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 24099_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 24099_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 96775_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 96775_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 35278_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 35278_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 65205_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 65205_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 28746_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 28746_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 111188_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 111188_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 69962_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 69962_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:19:07.36 +65:31:17.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 32575_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 32575_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 65663_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 65663_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 122716_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 122716_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:37:22.09 +65:16:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 1.960 2245486009899803904 309.34076268530 +65.27220485292 10.9928 10.0891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.960#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 46909_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 46909_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:26:54.19 +70:13:15.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 99736_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 99736_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 106362_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 106362_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 76725_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 76725_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 16262_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 16262_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:30:55.03 +73:29:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 4.455 2273880725887937920 322.72906101013 +73.48812458853 10.2904 8.8439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107966_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 107966_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:39:25.54 +67:58:26.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 122602_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 122602_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 20:46:01.72 +65:55:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.961 2245711061890014592 311.50525469842 +65.92780837682 12.2093 11.3600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 46561_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 46561_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 83447_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 83447_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:35:42.59 +68:39:08.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 111457_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 111457_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 54848_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 54848_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 50191_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 50191_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 122445_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 122445_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:36:27.00 +66:47:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 5.132 2212800381064167808 339.11511173196 +66.78740273431 12.2507 10.6124 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 122410_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 122410_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:49:18.21 +66:40:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.879 2212648717181046144 342.32928831904 +66.67520389553 13.3309 12.5823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31626_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 31626_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:16:18.05 +71:52:09.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54758_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 54758_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 107001_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 107001_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 31762_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 31762_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 50219_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 50219_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 74126_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 74126_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 101582_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 101582_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 110144_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 110144_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 46022_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 46022_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 35065_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 35065_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:51:16.89 +71:04:29.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104237_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 104237_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50594_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 50594_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72934_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 72934_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19127_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 19127_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33143_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 33143_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108755_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 108755_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82825_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 82825_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91239_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 91239_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44249_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 44249_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:47:00.74 +70:09:03.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41309_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 41309_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:28:40.14 +70:33:42.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33122_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 33122_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:41:55.74 +71:18:43.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23422_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 23422_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:43:03.58 +72:19:09.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39056_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 39056_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 22:10:37.40 +70:08:01.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34913_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 34913_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:06:23.41 +71:25:51.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96089_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079
The candidate 96089_Cep-04-Q2b1x1_2026-02-21_21-34-35_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 21:27:46.21 +66:48:36.6 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 41s
make_report_in_HTML.sh TOTAL: 485s
Prepared the HTML report for the field Cep-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:00:06.43 +74:35:21.9
21:20:33.74 +73:17:58.7
21:38:38.29 +73:03:03.8
21:20:47.91 +71:59:54.6
21:16:17.89 +71:52:09.3
21:57:33.79 +71:18:24.7
21:20:37.50 +71:31:11.0
21:51:16.86 +71:04:29.5
21:17:29.03 +70:30:50.9
21:26:54.18 +70:13:15.4
21:16:58.28 +70:15:44.2
22:26:55.72 +68:25:12.9
21:23:25.12 +69:08:59.2
22:31:29.97 +67:23:50.0
21:35:42.56 +68:39:08.6
21:39:10.31 +68:16:13.8
21:39:25.53 +67:58:26.2
21:44:42.07 +67:49:31.0
21:46:12.20 +67:38:13.5
21:28:06.02 +66:20:29.5
21:32:02.72 +65:09:50.2
21:45:28.22 +66:00:19.7
21:19:07.36 +65:31:18.3
22:32:58.85 +66:54:43.5
20:26:21.56 +66:28:43.2
20:39:55.26 +73:32:07.8
20:30:15.79 +66:44:12.1
20:29:33.52 +67:02:15.7
19:56:26.86 +73:36:58.5
20:01:16.49 +72:54:15.9
20:22:25.21 +70:03:41.4
20:27:22.59 +72:44:39.6
20:36:46.02 +65:25:39.3
20:14:32.22 +70:50:20.6
20:25:04.46 +72:56:16.7
20:25:26.70 +73:13:53.6
20:30:34.81 +65:27:11.2
20:13:51.87 +72:28:28.7
20:25:40.31 +64:47:48.0
20:03:01.33 +72:37:10.6
20:20:36.24 +66:09:01.0
19:54:15.53 +73:23:22.0
20:37:00.01 +65:15:24.6
20:23:50.97 +69:35:48.2
20:20:57.02 +73:41:09.9
23:00:10.28 +70:02:27.3
20:03:44.77 +71:36:25.5
20:36:38.77 +68:17:39.4
20:04:23.02 +71:45:46.6
20:49:42.41 +72:15:49.0
21:08:25.58 +74:43:29.6
21:40:31.74 +74:08:03.4
21:07:41.94 +67:34:32.9
21:46:37.15 +67:13:12.6
21:16:46.32 +67:40:14.9
21:04:16.01 +67:42:48.4
21:55:34.44 +67:08:08.4
21:57:47.10 +67:04:28.4
22:21:27.70 +66:26:45.2
21:52:21.70 +67:18:10.9
21:14:24.69 +67:59:10.0
21:55:41.98 +67:28:45.3
21:04:36.71 +68:10:12.0
20:55:46.97 +68:12:37.8
21:20:47.01 +68:08:38.4
21:40:08.63 +68:02:45.2
21:20:21.40 +68:18:04.2
21:51:12.86 +67:56:12.9
21:22:59.08 +68:21:09.7
21:41:47.77 +68:11:38.2
21:47:55.08 +68:12:32.6
21:39:12.14 +68:25:29.0
21:32:12.31 +74:00:38.2
22:05:47.84 +73:28:59.3
20:35:53.84 +74:35:02.3
20:26:22.96 +72:03:22.8
20:20:45.45 +70:42:26.9
20:10:07.32 +69:37:48.8
20:27:13.43 +65:44:51.3
20:22:54.55 +71:21:28.8
20:32:53.41 +64:50:36.0
20:24:48.92 +68:31:58.8
20:51:44.53 +65:12:30.1
19:59:46.26 +73:19:43.4
20:19:38.33 +67:00:13.0
20:23:23.83 +65:35:13.5
21:08:08.20 +73:56:04.0
20:02:42.43 +71:34:15.7
21:06:27.74 +64:59:50.8
21:57:48.17 +67:56:56.6
20:24:15.33 +67:12:31.1
21:27:46.01 +65:10:07.8
20:41:48.08 +65:27:05.6
20:43:09.53 +65:21:09.8
20:25:51.01 +66:05:13.4
20:16:35.23 +67:18:38.9
20:23:27.96 +66:01:10.9
20:16:51.72 +68:34:54.6
20:54:48.06 +65:03:49.9
20:04:24.40 +73:03:41.1
20:19:23.66 +66:32:14.4
20:28:21.38 +67:14:59.5
20:30:08.66 +66:47:01.5
21:48:28.57 +67:49:45.4
20:26:45.80 +67:26:55.8
20:14:11.83 +68:43:31.7
20:17:58.46 +67:19:00.6
20:38:57.00 +68:14:26.9
21:53:46.05 +69:03:54.2
20:19:06.67 +71:38:51.7
20:39:11.59 +65:31:13.9
20:18:53.99 +67:05:18.8
20:31:21.93 +67:03:47.4
20:21:45.72 +66:52:05.8
20:15:05.12 +68:06:40.0
20:34:38.76 +66:26:22.1
20:30:54.97 +66:38:55.6
20:32:05.58 +72:59:00.9
20:26:08.99 +67:44:09.2
20:21:58.79 +68:45:18.2
20:27:14.16 +67:13:17.7
20:25:34.69 +67:29:45.2
20:38:14.68 +65:49:47.4
20:15:27.47 +70:03:17.2
20:18:26.15 +73:37:09.6
20:38:42.14 +65:29:22.4
20:37:18.22 +64:54:39.8
20:21:40.33 +73:44:41.2
20:03:28.99 +72:51:43.8
20:13:19.13 +71:52:00.7
20:17:41.59 +72:28:52.0
20:01:44.40 +72:06:09.3
20:05:29.43 +71:39:22.0
20:19:29.80 +68:33:12.6
20:13:45.72 +71:31:44.4
20:25:41.87 +64:47:58.4
20:27:02.28 +69:55:32.6
20:21:41.24 +71:57:48.9
20:20:12.08 +69:06:04.5
20:19:27.23 +69:14:32.4
20:12:20.08 +71:09:34.7
19:52:59.70 +73:19:19.9
20:29:20.30 +65:10:13.0
20:29:00.01 +73:26:37.9
20:21:06.58 +71:07:52.6
20:23:17.51 +71:23:23.0
20:44:40.42 +65:35:08.2
20:23:04.05 +72:42:26.1
20:14:35.94 +71:38:05.2
20:14:32.15 +72:40:17.3
20:01:55.27 +72:51:00.7
20:24:59.79 +65:11:28.0
20:12:40.38 +70:15:02.5
19:55:02.31 +73:16:00.1
20:03:47.27 +71:52:53.9
20:10:23.34 +72:20:54.4
20:28:27.06 +74:01:30.0
20:18:42.22 +73:49:31.7
20:22:34.18 +73:11:29.5
20:09:32.12 +73:25:53.3
19:59:16.99 +73:33:21.4
19:59:13.12 +73:33:35.1
20:21:11.54 +70:20:32.7
20:03:36.79 +70:17:56.0
20:23:48.88 +73:30:27.0
20:03:01.62 +72:46:36.9
20:18:40.09 +68:52:26.1
20:18:53.53 +73:13:04.2
19:57:26.92 +73:21:20.6
20:30:45.05 +64:53:06.6
20:20:55.73 +72:14:23.8
20:12:46.83 +69:49:54.9
20:23:41.89 +73:45:15.7
20:16:11.53 +69:46:08.0
20:44:24.26 +65:08:24.0
20:12:02.76 +72:28:59.7
20:16:12.43 +69:46:10.5
21:48:42.03 +68:15:09.6
20:23:34.74 +72:19:48.6
20:02:41.06 +71:33:47.3
20:03:44.65 +73:12:47.0
20:20:13.06 +65:50:49.1
21:52:52.86 +69:03:51.1
19:56:20.86 +72:45:39.5
20:03:31.19 +70:29:17.7
22:35:41.14 +64:40:01.7
20:53:57.19 +65:32:08.1
19:59:38.86 +73:28:15.3
19:55:32.44 +73:14:48.3
20:03:26.43 +70:16:18.6
20:24:21.08 +64:54:57.6
20:41:55.67 +65:44:21.6
20:54:52.49 +65:53:47.2
20:41:39.76 +65:06:35.0
20:22:44.01 +65:30:16.7
22:15:54.07 +65:06:37.1
20:05:25.34 +73:26:03.6
20:29:02.10 +65:03:54.2
20:49:53.98 +74:31:35.6
20:44:10.40 +67:20:30.7
19:56:54.77 +72:55:15.2
20:19:26.45 +71:38:05.7
20:16:27.82 +66:48:30.4
20:23:24.73 +65:42:34.7
20:07:44.38 +69:25:31.1
20:28:47.46 +65:52:11.8
20:26:47.73 +64:50:46.9
22:46:00.15 +67:07:22.6
20:28:06.49 +65:41:43.7
22:55:56.82 +67:20:39.8
21:39:09.36 +73:29:25.4
20:56:13.48 +73:33:30.4
21:08:48.28 +73:26:07.7
21:02:07.89 +73:25:45.2
21:52:46.39 +72:58:34.7
21:25:02.83 +73:15:49.1
21:47:45.12 +72:57:46.7
20:27:55.97 +73:05:42.7
20:35:39.96 +73:00:07.3
22:19:51.58 +72:01:25.6
21:16:58.14 +72:45:17.3
22:06:11.90 +72:02:18.3
21:54:52.97 +72:10:40.9
21:18:15.27 +72:33:05.5
20:06:28.13 +71:56:42.9
21:53:16.19 +71:49:10.3
20:03:07.88 +71:38:47.7
22:03:00.53 +71:26:10.2
21:27:31.45 +71:48:57.4
22:45:07.94 +69:58:34.1
21:00:25.44 +71:50:23.1
22:11:50.28 +70:56:52.3
22:13:23.83 +70:51:08.0
20:57:12.42 +71:42:56.2
21:20:16.23 +71:35:19.6
20:56:08.33 +71:33:38.2
21:12:14.44 +71:32:36.7
20:59:50.59 +71:31:07.3
21:41:39.71 +71:10:04.0
22:02:06.31 +70:50:22.6
22:09:10.23 +70:26:17.9
22:00:42.55 +70:37:56.1
22:01:32.82 +70:34:12.3
21:38:44.92 +70:56:59.3
22:09:49.30 +70:18:31.1
21:12:13.98 +71:03:50.3
22:07:35.06 +70:08:20.1
21:40:03.24 +70:32:41.7
21:41:55.66 +70:25:49.3
22:34:35.47 +69:06:22.7
22:24:58.64 +69:20:32.9
22:20:41.64 +69:23:35.9
21:18:50.66 +70:28:29.3
21:30:22.78 +70:19:28.3
21:13:19.28 +70:24:05.7
21:42:52.00 +69:55:15.2
21:54:53.46 +69:42:29.0
21:17:35.63 +70:04:34.1
21:29:21.82 +69:58:38.2
22:04:31.85 +69:21:23.4
21:02:14.59 +70:07:19.3
21:06:45.86 +70:04:20.3
21:26:27.43 +69:56:56.6
20:58:42.10 +70:03:25.5
21:37:17.20 +69:47:52.2
22:07:23.95 +69:04:10.5
21:50:30.84 +69:17:46.9
21:39:33.81 +69:28:37.5
21:40:06.91 +69:27:57.8
21:55:24.66 +69:11:15.6
21:46:22.69 +69:11:06.8
21:54:34.71 +68:48:26.7
21:16:14.25 +69:12:27.0
22:08:26.36 +68:18:10.5
21:43:21.59 +68:53:19.2
21:32:55.57 +69:00:00.2
21:11:51.02 +65:10:27.7
20:35:36.69 +65:09:04.9
21:46:14.01 +64:53:57.3
20:41:11.29 +65:24:06.7
21:39:42.82 +65:15:31.9
22:05:23.09 +64:41:46.0
20:22:03.05 +65:25:14.7
21:57:34.51 +65:02:12.5
21:22:03.34 +65:41:36.6
21:31:28.87 +65:35:29.6
22:16:44.98 +66:59:41.9
21:41:32.29 +67:52:48.4
21:32:05.49 +68:03:34.6
22:43:06.17 +66:08:59.0
22:40:35.93 +66:30:39.0
22:00:26.71 +67:59:46.7
21:27:49.06 +65:40:02.5
21:29:00.12 +65:39:26.0
20:19:19.83 +66:04:25.8
20:55:10.51 +67:02:00.4
20:48:27.25 +67:05:04.6
21:33:24.17 +66:57:46.7
21:36:29.20 +68:33:35.1
21:36:28.07 +68:43:42.6
21:49:51.61 +68:31:23.7
22:32:12.21 +67:18:10.0
20:32:42.06 +68:55:05.8
22:00:43.17 +65:03:51.0
21:33:19.56 +65:43:30.0
22:22:18.59 +64:29:43.9
21:39:14.96 +65:43:35.8
21:29:10.18 +66:13:07.9
22:07:35.53 +67:10:49.1
21:58:22.06 +65:57:05.5
21:53:17.88 +66:04:52.8
21:40:30.50 +66:26:04.9
21:00:12.28 +66:54:45.3
21:47:36.52 +66:28:37.0
21:41:16.39 +66:40:55.9
21:44:03.52 +66:39:14.1
21:04:54.54 +67:08:11.9
21:58:03.96 +66:28:13.7
21:41:44.97 +66:52:46.6
21:04:26.49 +67:16:07.2
21:54:36.34 +66:45:26.6
########### Completed Cep-04-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 ####
20:26:21.56 +66:28:43.2
20:39:55.26 +73:32:07.8
20:30:15.79 +66:44:12.1
20:29:33.52 +67:02:15.7
19:56:26.86 +73:36:58.5
20:01:16.49 +72:54:15.9
20:22:25.21 +70:03:41.4
20:27:22.59 +72:44:39.6
20:36:46.02 +65:25:39.3
20:14:32.22 +70:50:20.6
20:25:04.46 +72:56:16.7
20:25:26.70 +73:13:53.6
20:30:34.81 +65:27:11.2
20:13:51.87 +72:28:28.7
20:25:40.31 +64:47:48.0
20:03:01.33 +72:37:10.6
20:20:36.24 +66:09:01.0
19:54:15.53 +73:23:22.0
20:37:00.01 +65:15:24.6
20:23:50.97 +69:35:48.2
20:20:57.02 +73:41:09.9
23:00:10.28 +70:02:27.3
20:03:44.77 +71:36:25.5
20:36:38.77 +68:17:39.4
20:04:23.02 +71:45:46.6
20:49:42.41 +72:15:49.0
21:51:16.86 +71:04:29.5
22:32:58.85 +66:54:43.5
21:35:42.56 +68:39:08.6
21:32:02.72 +65:09:50.2
21:28:06.02 +66:20:29.5
21:26:54.18 +70:13:15.4
21:44:42.07 +67:49:31.0
21:23:25.12 +69:08:59.2
21:57:33.79 +71:18:24.7
22:26:55.72 +68:25:12.9
21:45:28.22 +66:00:19.7
21:16:58.28 +70:15:44.2
21:17:29.03 +70:30:50.9
21:20:47.91 +71:59:54.6
21:38:38.29 +73:03:03.8
21:39:10.31 +68:16:13.8
22:31:29.97 +67:23:50.0
21:19:07.36 +65:31:18.3
21:00:06.43 +74:35:21.9
21:20:33.74 +73:17:58.7
21:16:17.89 +71:52:09.3
21:39:25.53 +67:58:26.2
21:46:12.20 +67:38:13.5
21:20:37.50 +71:31:11.0
20:35:53.84 +74:35:02.3
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20:20:45.45 +70:42:26.9
20:10:07.32 +69:37:48.8
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20:32:53.41 +64:50:36.0
20:24:48.92 +68:31:58.8
20:51:44.53 +65:12:30.1
19:59:46.26 +73:19:43.4
20:19:38.33 +67:00:13.0
20:23:23.83 +65:35:13.5
21:08:08.20 +73:56:04.0
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21:57:48.17 +67:56:56.6
20:24:15.33 +67:12:31.1
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20:43:09.53 +65:21:09.8
20:25:51.01 +66:05:13.4
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20:23:27.96 +66:01:10.9
20:16:51.72 +68:34:54.6
20:54:48.06 +65:03:49.9
20:04:24.40 +73:03:41.1
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20:30:08.66 +66:47:01.5
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20:14:11.83 +68:43:31.7
20:17:58.46 +67:19:00.6
20:38:57.00 +68:14:26.9
21:53:46.05 +69:03:54.2
20:19:06.67 +71:38:51.7
20:39:11.59 +65:31:13.9
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20:31:21.93 +67:03:47.4
20:21:45.72 +66:52:05.8
20:15:05.12 +68:06:40.0
20:34:38.76 +66:26:22.1
20:30:54.97 +66:38:55.6
20:32:05.58 +72:59:00.9
20:26:08.99 +67:44:09.2
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20:27:14.16 +67:13:17.7
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20:38:14.68 +65:49:47.4
20:15:27.47 +70:03:17.2
20:18:26.15 +73:37:09.6
20:38:42.14 +65:29:22.4
20:37:18.22 +64:54:39.8
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20:13:19.13 +71:52:00.7
20:17:41.59 +72:28:52.0
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20:19:29.80 +68:33:12.6
20:13:45.72 +71:31:44.4
20:25:41.87 +64:47:58.4
20:27:02.28 +69:55:32.6
20:21:41.24 +71:57:48.9
20:20:12.08 +69:06:04.5
20:19:27.23 +69:14:32.4
20:12:20.08 +71:09:34.7
19:52:59.70 +73:19:19.9
20:29:20.30 +65:10:13.0
20:29:00.01 +73:26:37.9
20:21:06.58 +71:07:52.6
20:23:17.51 +71:23:23.0
20:44:40.42 +65:35:08.2
20:23:04.05 +72:42:26.1
20:14:35.94 +71:38:05.2
20:14:32.15 +72:40:17.3
20:01:55.27 +72:51:00.7
20:24:59.79 +65:11:28.0
20:12:40.38 +70:15:02.5
19:55:02.31 +73:16:00.1
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20:10:23.34 +72:20:54.4
20:28:27.06 +74:01:30.0
20:18:42.22 +73:49:31.7
20:22:34.18 +73:11:29.5
20:09:32.12 +73:25:53.3
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19:59:13.12 +73:33:35.1
20:21:11.54 +70:20:32.7
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20:03:01.62 +72:46:36.9
20:18:40.09 +68:52:26.1
20:18:53.53 +73:13:04.2
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20:30:45.05 +64:53:06.6
20:20:55.73 +72:14:23.8
20:12:46.83 +69:49:54.9
20:23:41.89 +73:45:15.7
20:16:11.53 +69:46:08.0
20:44:24.26 +65:08:24.0
20:12:02.76 +72:28:59.7
20:16:12.43 +69:46:10.5
21:48:42.03 +68:15:09.6
20:23:34.74 +72:19:48.6
20:02:41.06 +71:33:47.3
20:03:44.65 +73:12:47.0
20:20:13.06 +65:50:49.1
21:52:52.86 +69:03:51.1
19:56:20.86 +72:45:39.5
20:03:31.19 +70:29:17.7
22:35:41.14 +64:40:01.7
20:53:57.19 +65:32:08.1
19:59:38.86 +73:28:15.3
19:55:32.44 +73:14:48.3
20:03:26.43 +70:16:18.6
20:24:21.08 +64:54:57.6
20:41:55.67 +65:44:21.6
20:54:52.49 +65:53:47.2
20:41:39.76 +65:06:35.0
20:22:44.01 +65:30:16.7
22:15:54.07 +65:06:37.1
20:05:25.34 +73:26:03.6
20:29:02.10 +65:03:54.2
20:49:53.98 +74:31:35.6
20:44:10.40 +67:20:30.7
19:56:54.77 +72:55:15.2
20:19:26.45 +71:38:05.7
20:16:27.82 +66:48:30.4
20:23:24.73 +65:42:34.7
20:07:44.38 +69:25:31.1
20:28:47.46 +65:52:11.8
20:26:47.73 +64:50:46.9
22:46:00.15 +67:07:22.6
20:28:06.49 +65:41:43.7
22:55:56.82 +67:20:39.8
22:00:42.55 +70:37:56.1
21:26:27.43 +69:56:56.6
21:50:30.84 +69:17:46.9
21:00:25.44 +71:50:23.1
21:42:52.00 +69:55:15.2
20:19:19.83 +66:04:25.8
21:47:45.12 +72:57:46.7
21:17:35.63 +70:04:34.1
21:55:34.44 +67:08:08.4
22:07:23.95 +69:04:10.5
21:18:15.27 +72:33:05.5
21:40:08.63 +68:02:45.2
22:09:49.30 +70:18:31.1
21:04:54.54 +67:08:11.9
21:04:26.49 +67:16:07.2
21:33:24.17 +66:57:46.7
20:32:42.06 +68:55:05.8
21:54:53.46 +69:42:29.0
22:34:35.47 +69:06:22.7
21:38:44.92 +70:56:59.3
21:44:03.52 +66:39:14.1
21:46:37.15 +67:13:12.6
21:08:25.58 +74:43:29.6
21:32:05.49 +68:03:34.6
20:41:11.29 +65:24:06.7
21:46:22.69 +69:11:06.8
22:05:23.09 +64:41:46.0
21:02:07.89 +73:25:45.2
20:56:13.48 +73:33:30.4
21:40:30.50 +66:26:04.9
22:00:43.17 +65:03:51.0
21:57:34.51 +65:02:12.5
22:32:12.21 +67:18:10.0
21:58:22.06 +65:57:05.5
21:12:14.44 +71:32:36.7
21:27:31.45 +71:48:57.4
21:39:14.96 +65:43:35.8
20:58:42.10 +70:03:25.5
22:40:35.93 +66:30:39.0
22:07:35.06 +70:08:20.1
21:12:13.98 +71:03:50.3
21:39:09.36 +73:29:25.4
21:39:33.81 +69:28:37.5
21:41:44.97 +66:52:46.6
22:06:11.90 +72:02:18.3
21:20:47.01 +68:08:38.4
21:40:31.74 +74:08:03.4
21:14:24.69 +67:59:10.0
21:52:46.39 +72:58:34.7
21:53:17.88 +66:04:52.8
21:54:34.71 +68:48:26.7
21:32:55.57 +69:00:00.2
21:29:21.82 +69:58:38.2
21:58:03.96 +66:28:13.7
20:59:50.59 +71:31:07.3
20:55:10.51 +67:02:00.4
21:16:14.25 +69:12:27.0
21:04:36.71 +68:10:12.0
20:35:39.96 +73:00:07.3
21:36:28.07 +68:43:42.6
21:00:12.28 +66:54:45.3
21:31:28.87 +65:35:29.6
20:27:55.97 +73:05:42.7
22:03:00.53 +71:26:10.2
20:22:03.05 +65:25:14.7
22:24:58.64 +69:20:32.9
21:33:19.56 +65:43:30.0
20:57:12.42 +71:42:56.2
21:16:46.32 +67:40:14.9
21:41:32.29 +67:52:48.4
21:51:12.86 +67:56:12.9
21:27:49.06 +65:40:02.5
21:39:42.82 +65:15:31.9
21:08:48.28 +73:26:07.7
22:02:06.31 +70:50:22.6
21:20:16.23 +71:35:19.6
20:03:07.88 +71:38:47.7
21:37:17.20 +69:47:52.2
22:09:10.23 +70:26:17.9
21:18:50.66 +70:28:29.3
22:08:26.36 +68:18:10.5
22:07:35.53 +67:10:49.1
20:06:28.13 +71:56:42.9
22:43:06.17 +66:08:59.0
21:22:59.08 +68:21:09.7
22:21:27.70 +66:26:45.2
22:19:51.58 +72:01:25.6
21:40:03.24 +70:32:41.7
20:56:08.33 +71:33:38.2
21:32:12.31 +74:00:38.2
21:43:21.59 +68:53:19.2
21:47:36.52 +66:28:37.0
21:49:51.61 +68:31:23.7
22:01:32.82 +70:34:12.3
22:20:41.64 +69:23:35.9
22:22:18.59 +64:29:43.9
21:41:55.66 +70:25:49.3
21:57:47.10 +67:04:28.4
22:00:26.71 +67:59:46.7
22:05:47.84 +73:28:59.3
20:48:27.25 +67:05:04.6
21:22:03.34 +65:41:36.6
21:54:52.97 +72:10:40.9
21:04:16.01 +67:42:48.4
21:46:14.01 +64:53:57.3
21:16:58.14 +72:45:17.3
21:41:16.39 +66:40:55.9
21:41:39.71 +71:10:04.0
21:11:51.02 +65:10:27.7
21:53:16.19 +71:49:10.3
21:47:55.08 +68:12:32.6
22:11:50.28 +70:56:52.3
20:35:36.69 +65:09:04.9
21:54:36.34 +66:45:26.6
21:55:41.98 +67:28:45.3
21:29:00.12 +65:39:26.0
21:13:19.28 +70:24:05.7
21:39:12.14 +68:25:29.0
21:55:24.66 +69:11:15.6
22:04:31.85 +69:21:23.4
21:40:06.91 +69:27:57.8
20:55:46.97 +68:12:37.8
22:45:07.94 +69:58:34.1
21:02:14.59 +70:07:19.3
21:07:41.94 +67:34:32.9
21:41:47.77 +68:11:38.2
21:30:22.78 +70:19:28.3
21:52:21.70 +67:18:10.9
21:06:45.86 +70:04:20.3
22:16:44.98 +66:59:41.9
21:25:02.83 +73:15:49.1
22:13:23.83 +70:51:08.0
21:20:21.40 +68:18:04.2
21:36:29.20 +68:33:35.1
21:29:10.18 +66:13:07.9
###################################################################################
20:26:21.56 +66:28:43.2 -- not an asteroid (will add it to exclusion list)
20:39:55.26 +73:32:07.8 -- not an asteroid (will add it to exclusion list)
20:30:15.79 +66:44:12.1 -- not an asteroid (will add it to exclusion list)
20:29:33.52 +67:02:15.7 -- not an asteroid (will add it to exclusion list)
19:56:26.86 +73:36:58.5 -- not an asteroid (will add it to exclusion list)
20:01:16.49 +72:54:15.9 -- not an asteroid (will add it to exclusion list)
20:22:25.21 +70:03:41.4 -- not an asteroid (will add it to exclusion list)
20:27:22.59 +72:44:39.6 -- not an asteroid (will add it to exclusion list)
20:36:46.02 +65:25:39.3 -- not an asteroid (will add it to exclusion list)
20:14:32.22 +70:50:20.6 -- not an asteroid (will add it to exclusion list)
20:25:04.46 +72:56:16.7 -- not an asteroid (will add it to exclusion list)
20:25:26.70 +73:13:53.6 -- not an asteroid (will add it to exclusion list)
20:30:34.81 +65:27:11.2 -- not an asteroid (will add it to exclusion list)
20:13:51.87 +72:28:28.7 -- not an asteroid (will add it to exclusion list)
20:25:40.31 +64:47:48.0 -- not an asteroid (will add it to exclusion list)
20:03:01.33 +72:37:10.6 -- not an asteroid (will add it to exclusion list)
20:20:36.24 +66:09:01.0 -- not an asteroid (will add it to exclusion list)
19:54:15.53 +73:23:22.0 -- not an asteroid (will add it to exclusion list)
20:37:00.01 +65:15:24.6 -- not an asteroid (will add it to exclusion list)
20:23:50.97 +69:35:48.2 -- not an asteroid (will add it to exclusion list)
20:20:57.02 +73:41:09.9 -- not an asteroid (will add it to exclusion list)
23:00:10.28 +70:02:27.3 -- not an asteroid (will add it to exclusion list)
20:03:44.77 +71:36:25.5 -- not an asteroid (will add it to exclusion list)
20:36:38.77 +68:17:39.4 -- not an asteroid (will add it to exclusion list)
20:04:23.02 +71:45:46.6 -- not an asteroid (will add it to exclusion list)
20:49:42.41 +72:15:49.0 -- not an asteroid (will add it to exclusion list)
21:51:16.86 +71:04:29.5 -- not an asteroid (will add it to exclusion list)
22:32:58.85 +66:54:43.5 -- not an asteroid (will add it to exclusion list)
21:35:42.56 +68:39:08.6 -- not an asteroid (will add it to exclusion list)
21:32:02.72 +65:09:50.2 -- not an asteroid (will add it to exclusion list)
21:28:06.02 +66:20:29.5 -- not an asteroid (will add it to exclusion list)
21:26:54.18 +70:13:15.4 -- not an asteroid (will add it to exclusion list)
21:44:42.07 +67:49:31.0 -- not an asteroid (will add it to exclusion list)
21:23:25.12 +69:08:59.2 -- not an asteroid (will add it to exclusion list)
21:57:33.79 +71:18:24.7 -- not an asteroid (will add it to exclusion list)
22:26:55.72 +68:25:12.9 -- not an asteroid (will add it to exclusion list)
21:45:28.22 +66:00:19.7 -- not an asteroid (will add it to exclusion list)
21:16:58.28 +70:15:44.2 -- not an asteroid (will add it to exclusion list)
21:17:29.03 +70:30:50.9 -- not an asteroid (will add it to exclusion list)
21:20:47.91 +71:59:54.6 -- not an asteroid (will add it to exclusion list)
21:38:38.29 +73:03:03.8 -- not an asteroid (will add it to exclusion list)
21:39:10.31 +68:16:13.8 -- not an asteroid (will add it to exclusion list)
22:31:29.97 +67:23:50.0 -- not an asteroid (will add it to exclusion list)
21:19:07.36 +65:31:18.3 -- not an asteroid (will add it to exclusion list)
21:00:06.43 +74:35:21.9 -- not an asteroid (will add it to exclusion list)
21:20:33.74 +73:17:58.7 -- not an asteroid (will add it to exclusion list)
21:16:17.89 +71:52:09.3 -- not an asteroid (will add it to exclusion list)
21:39:25.53 +67:58:26.2 -- not an asteroid (will add it to exclusion list)
21:46:12.20 +67:38:13.5 -- not an asteroid (will add it to exclusion list)
21:20:37.50 +71:31:11.0 -- not an asteroid (will add it to exclusion list)
20:35:53.84 +74:35:02.3 -- not an asteroid (will add it to exclusion list)
20:26:22.96 +72:03:22.8 -- not an asteroid (will add it to exclusion list)
20:20:45.45 +70:42:26.9 -- not an asteroid (will add it to exclusion list)
20:10:07.32 +69:37:48.8 -- not an asteroid (will add it to exclusion list)
20:27:13.43 +65:44:51.3 -- not an asteroid (will add it to exclusion list)
20:22:54.55 +71:21:28.8 -- not an asteroid (will add it to exclusion list)
20:32:53.41 +64:50:36.0 -- not an asteroid (will add it to exclusion list)
20:24:48.92 +68:31:58.8 -- not an asteroid (will add it to exclusion list)
20:51:44.53 +65:12:30.1 -- not an asteroid (will add it to exclusion list)
19:59:46.26 +73:19:43.4 -- not an asteroid (will add it to exclusion list)
20:19:38.33 +67:00:13.0 -- not an asteroid (will add it to exclusion list)
20:23:23.83 +65:35:13.5 -- not an asteroid (will add it to exclusion list)
21:08:08.20 +73:56:04.0 -- not an asteroid (will add it to exclusion list)
20:02:42.43 +71:34:15.7 -- not an asteroid (will add it to exclusion list)
21:06:27.74 +64:59:50.8 -- not an asteroid (will add it to exclusion list)
21:57:48.17 +67:56:56.6 -- not an asteroid (will add it to exclusion list)
20:24:15.33 +67:12:31.1 -- not an asteroid (will add it to exclusion list)
21:27:46.01 +65:10:07.8 -- not an asteroid (will add it to exclusion list)
20:41:48.08 +65:27:05.6 -- not an asteroid (will add it to exclusion list)
20:43:09.53 +65:21:09.8 -- not an asteroid (will add it to exclusion list)
20:25:51.01 +66:05:13.4 -- not an asteroid (will add it to exclusion list)
20:16:35.23 +67:18:38.9 -- not an asteroid (will add it to exclusion list)
20:23:27.96 +66:01:10.9 -- not an asteroid (will add it to exclusion list)
20:16:51.72 +68:34:54.6 -- not an asteroid (will add it to exclusion list)
20:54:48.06 +65:03:49.9 -- not an asteroid (will add it to exclusion list)
20:04:24.40 +73:03:41.1 -- not an asteroid (will add it to exclusion list)
20:19:23.66 +66:32:14.4 -- not an asteroid (will add it to exclusion list)
20:28:21.38 +67:14:59.5 -- not an asteroid (will add it to exclusion list)
20:30:08.66 +66:47:01.5 -- not an asteroid (will add it to exclusion list)
21:48:28.57 +67:49:45.4 -- not an asteroid (will add it to exclusion list)
20:26:45.80 +67:26:55.8 -- not an asteroid (will add it to exclusion list)
20:14:11.83 +68:43:31.7 -- not an asteroid (will add it to exclusion list)
20:17:58.46 +67:19:00.6 -- not an asteroid (will add it to exclusion list)
20:38:57.00 +68:14:26.9 -- not an asteroid (will add it to exclusion list)
21:53:46.05 +69:03:54.2 -- not an asteroid (will add it to exclusion list)
20:19:06.67 +71:38:51.7 -- not an asteroid (will add it to exclusion list)
20:39:11.59 +65:31:13.9 -- not an asteroid (will add it to exclusion list)
20:18:53.99 +67:05:18.8 -- not an asteroid (will add it to exclusion list)
20:31:21.93 +67:03:47.4 -- not an asteroid (will add it to exclusion list)
20:21:45.72 +66:52:05.8 -- not an asteroid (will add it to exclusion list)
20:15:05.12 +68:06:40.0 -- not an asteroid (will add it to exclusion list)
20:34:38.76 +66:26:22.1 -- not an asteroid (will add it to exclusion list)
20:30:54.97 +66:38:55.6 -- not an asteroid (will add it to exclusion list)
20:32:05.58 +72:59:00.9 -- not an asteroid (will add it to exclusion list)
20:26:08.99 +67:44:09.2 -- not an asteroid (will add it to exclusion list)
20:21:58.79 +68:45:18.2 -- not an asteroid (will add it to exclusion list)
20:27:14.16 +67:13:17.7 -- not an asteroid (will add it to exclusion list)
20:25:34.69 +67:29:45.2 -- not an asteroid (will add it to exclusion list)
20:38:14.68 +65:49:47.4 -- not an asteroid (will add it to exclusion list)
20:15:27.47 +70:03:17.2 -- not an asteroid (will add it to exclusion list)
20:18:26.15 +73:37:09.6 -- not an asteroid (will add it to exclusion list)
20:38:42.14 +65:29:22.4 -- not an asteroid (will add it to exclusion list)
20:37:18.22 +64:54:39.8 -- not an asteroid (will add it to exclusion list)
20:21:40.33 +73:44:41.2 -- not an asteroid (will add it to exclusion list)
20:03:28.99 +72:51:43.8 -- not an asteroid (will add it to exclusion list)
20:13:19.13 +71:52:00.7 -- not an asteroid (will add it to exclusion list)
20:17:41.59 +72:28:52.0 -- not an asteroid (will add it to exclusion list)
20:01:44.40 +72:06:09.3 -- not an asteroid (will add it to exclusion list)
20:05:29.43 +71:39:22.0 -- not an asteroid (will add it to exclusion list)
20:19:29.80 +68:33:12.6 -- not an asteroid (will add it to exclusion list)
20:13:45.72 +71:31:44.4 -- not an asteroid (will add it to exclusion list)
20:25:41.87 +64:47:58.4 -- not an asteroid (will add it to exclusion list)
20:27:02.28 +69:55:32.6 -- not an asteroid (will add it to exclusion list)
20:21:41.24 +71:57:48.9 -- not an asteroid (will add it to exclusion list)
20:20:12.08 +69:06:04.5 -- not an asteroid (will add it to exclusion list)
20:19:27.23 +69:14:32.4 -- not an asteroid (will add it to exclusion list)
20:12:20.08 +71:09:34.7 -- not an asteroid (will add it to exclusion list)
19:52:59.70 +73:19:19.9 -- not an asteroid (will add it to exclusion list)
20:29:20.30 +65:10:13.0 -- not an asteroid (will add it to exclusion list)
20:29:00.01 +73:26:37.9 -- not an asteroid (will add it to exclusion list)
20:21:06.58 +71:07:52.6 -- not an asteroid (will add it to exclusion list)
20:23:17.51 +71:23:23.0 -- not an asteroid (will add it to exclusion list)
20:44:40.42 +65:35:08.2 -- not an asteroid (will add it to exclusion list)
20:23:04.05 +72:42:26.1 -- not an asteroid (will add it to exclusion list)
20:14:35.94 +71:38:05.2 -- not an asteroid (will add it to exclusion list)
20:14:32.15 +72:40:17.3 -- not an asteroid (will add it to exclusion list)
20:01:55.27 +72:51:00.7 -- not an asteroid (will add it to exclusion list)
20:24:59.79 +65:11:28.0 -- not an asteroid (will add it to exclusion list)
20:12:40.38 +70:15:02.5 -- not an asteroid (will add it to exclusion list)
19:55:02.31 +73:16:00.1 -- not an asteroid (will add it to exclusion list)
20:03:47.27 +71:52:53.9 -- not an asteroid (will add it to exclusion list)
20:10:23.34 +72:20:54.4 -- not an asteroid (will add it to exclusion list)
20:28:27.06 +74:01:30.0 -- not an asteroid (will add it to exclusion list)
20:18:42.22 +73:49:31.7 -- not an asteroid (will add it to exclusion list)
20:22:34.18 +73:11:29.5 -- not an asteroid (will add it to exclusion list)
20:09:32.12 +73:25:53.3 -- not an asteroid (will add it to exclusion list)
19:59:16.99 +73:33:21.4 -- not an asteroid (will add it to exclusion list)
19:59:13.12 +73:33:35.1 -- not an asteroid (will add it to exclusion list)
20:21:11.54 +70:20:32.7 -- not an asteroid (will add it to exclusion list)
20:03:36.79 +70:17:56.0 -- not an asteroid (will add it to exclusion list)
20:23:48.88 +73:30:27.0 -- not an asteroid (will add it to exclusion list)
20:03:01.62 +72:46:36.9 -- not an asteroid (will add it to exclusion list)
20:18:40.09 +68:52:26.1 -- not an asteroid (will add it to exclusion list)
20:18:53.53 +73:13:04.2 -- not an asteroid (will add it to exclusion list)
19:57:26.92 +73:21:20.6 -- not an asteroid (will add it to exclusion list)
20:30:45.05 +64:53:06.6 -- not an asteroid (will add it to exclusion list)
20:20:55.73 +72:14:23.8 -- not an asteroid (will add it to exclusion list)
20:12:46.83 +69:49:54.9 -- not an asteroid (will add it to exclusion list)
20:23:41.89 +73:45:15.7 -- not an asteroid (will add it to exclusion list)
20:16:11.53 +69:46:08.0 -- not an asteroid (will add it to exclusion list)
20:44:24.26 +65:08:24.0 -- not an asteroid (will add it to exclusion list)
20:12:02.76 +72:28:59.7 -- not an asteroid (will add it to exclusion list)
20:16:12.43 +69:46:10.5 -- not an asteroid (will add it to exclusion list)
21:48:42.03 +68:15:09.6 -- not an asteroid (will add it to exclusion list)
20:23:34.74 +72:19:48.6 -- not an asteroid (will add it to exclusion list)
20:02:41.06 +71:33:47.3 -- not an asteroid (will add it to exclusion list)
20:03:44.65 +73:12:47.0 -- not an asteroid (will add it to exclusion list)
20:20:13.06 +65:50:49.1 -- not an asteroid (will add it to exclusion list)
21:52:52.86 +69:03:51.1 -- not an asteroid (will add it to exclusion list)
19:56:20.86 +72:45:39.5 -- not an asteroid (will add it to exclusion list)
20:03:31.19 +70:29:17.7 -- not an asteroid (will add it to exclusion list)
22:35:41.14 +64:40:01.7 -- not an asteroid (will add it to exclusion list)
20:53:57.19 +65:32:08.1 -- not an asteroid (will add it to exclusion list)
19:59:38.86 +73:28:15.3 -- not an asteroid (will add it to exclusion list)
19:55:32.44 +73:14:48.3 -- not an asteroid (will add it to exclusion list)
20:03:26.43 +70:16:18.6 -- not an asteroid (will add it to exclusion list)
20:24:21.08 +64:54:57.6 -- not an asteroid (will add it to exclusion list)
20:41:55.67 +65:44:21.6 -- not an asteroid (will add it to exclusion list)
20:54:52.49 +65:53:47.2 -- not an asteroid (will add it to exclusion list)
20:41:39.76 +65:06:35.0 -- not an asteroid (will add it to exclusion list)
20:22:44.01 +65:30:16.7 -- not an asteroid (will add it to exclusion list)
22:15:54.07 +65:06:37.1 -- not an asteroid (will add it to exclusion list)
20:05:25.34 +73:26:03.6 -- not an asteroid (will add it to exclusion list)
20:29:02.10 +65:03:54.2 -- not an asteroid (will add it to exclusion list)
20:49:53.98 +74:31:35.6 -- not an asteroid (will add it to exclusion list)
20:44:10.40 +67:20:30.7 -- not an asteroid (will add it to exclusion list)
19:56:54.77 +72:55:15.2 -- not an asteroid (will add it to exclusion list)
20:19:26.45 +71:38:05.7 -- not an asteroid (will add it to exclusion list)
20:16:27.82 +66:48:30.4 -- not an asteroid (will add it to exclusion list)
20:23:24.73 +65:42:34.7 -- not an asteroid (will add it to exclusion list)
20:07:44.38 +69:25:31.1 -- not an asteroid (will add it to exclusion list)
20:28:47.46 +65:52:11.8 -- not an asteroid (will add it to exclusion list)
20:26:47.73 +64:50:46.9 -- not an asteroid (will add it to exclusion list)
22:46:00.15 +67:07:22.6 -- not an asteroid (will add it to exclusion list)
20:28:06.49 +65:41:43.7 -- not an asteroid (will add it to exclusion list)
22:55:56.82 +67:20:39.8 -- not an asteroid (will add it to exclusion list)
22:00:42.55 +70:37:56.1 -- not an asteroid (will add it to exclusion list)
21:26:27.43 +69:56:56.6 -- not an asteroid (will add it to exclusion list)
21:50:30.84 +69:17:46.9 -- not an asteroid (will add it to exclusion list)
21:00:25.44 +71:50:23.1 -- not an asteroid (will add it to exclusion list)
21:42:52.00 +69:55:15.2 -- not an asteroid (will add it to exclusion list)
20:19:19.83 +66:04:25.8 -- not an asteroid (will add it to exclusion list)
21:47:45.12 +72:57:46.7 -- not an asteroid (will add it to exclusion list)
21:17:35.63 +70:04:34.1 -- not an asteroid (will add it to exclusion list)
21:55:34.44 +67:08:08.4 -- not an asteroid (will add it to exclusion list)
22:07:23.95 +69:04:10.5 -- not an asteroid (will add it to exclusion list)
21:18:15.27 +72:33:05.5 -- not an asteroid (will add it to exclusion list)
21:40:08.63 +68:02:45.2 -- not an asteroid (will add it to exclusion list)
22:09:49.30 +70:18:31.1 -- not an asteroid (will add it to exclusion list)
21:04:54.54 +67:08:11.9 -- not an asteroid (will add it to exclusion list)
21:04:26.49 +67:16:07.2 -- not an asteroid (will add it to exclusion list)
21:33:24.17 +66:57:46.7 -- not an asteroid (will add it to exclusion list)
20:32:42.06 +68:55:05.8 -- not an asteroid (will add it to exclusion list)
21:54:53.46 +69:42:29.0 -- not an asteroid (will add it to exclusion list)
22:34:35.47 +69:06:22.7 -- not an asteroid (will add it to exclusion list)
21:38:44.92 +70:56:59.3 -- not an asteroid (will add it to exclusion list)
21:44:03.52 +66:39:14.1 -- not an asteroid (will add it to exclusion list)
21:46:37.15 +67:13:12.6 -- not an asteroid (will add it to exclusion list)
21:08:25.58 +74:43:29.6 -- not an asteroid (will add it to exclusion list)
21:32:05.49 +68:03:34.6 -- not an asteroid (will add it to exclusion list)
20:41:11.29 +65:24:06.7 -- not an asteroid (will add it to exclusion list)
21:46:22.69 +69:11:06.8 -- not an asteroid (will add it to exclusion list)
22:05:23.09 +64:41:46.0 -- not an asteroid (will add it to exclusion list)
21:02:07.89 +73:25:45.2 -- not an asteroid (will add it to exclusion list)
20:56:13.48 +73:33:30.4 -- not an asteroid (will add it to exclusion list)
21:40:30.50 +66:26:04.9 -- not an asteroid (will add it to exclusion list)
22:00:43.17 +65:03:51.0 -- not an asteroid (will add it to exclusion list)
21:57:34.51 +65:02:12.5 -- not an asteroid (will add it to exclusion list)
22:32:12.21 +67:18:10.0 -- not an asteroid (will add it to exclusion list)
21:58:22.06 +65:57:05.5 -- not an asteroid (will add it to exclusion list)
21:12:14.44 +71:32:36.7 -- not an asteroid (will add it to exclusion list)
21:27:31.45 +71:48:57.4 -- not an asteroid (will add it to exclusion list)
21:39:14.96 +65:43:35.8 -- not an asteroid (will add it to exclusion list)
20:58:42.10 +70:03:25.5 -- not an asteroid (will add it to exclusion list)
22:40:35.93 +66:30:39.0 -- not an asteroid (will add it to exclusion list)
22:07:35.06 +70:08:20.1 -- not an asteroid (will add it to exclusion list)
21:12:13.98 +71:03:50.3 -- not an asteroid (will add it to exclusion list)
21:39:09.36 +73:29:25.4 -- not an asteroid (will add it to exclusion list)
21:39:33.81 +69:28:37.5 -- not an asteroid (will add it to exclusion list)
21:41:44.97 +66:52:46.6 -- not an asteroid (will add it to exclusion list)
22:06:11.90 +72:02:18.3 -- not an asteroid (will add it to exclusion list)
21:20:47.01 +68:08:38.4 -- not an asteroid (will add it to exclusion list)
21:40:31.74 +74:08:03.4 -- not an asteroid (will add it to exclusion list)
21:14:24.69 +67:59:10.0 -- not an asteroid (will add it to exclusion list)
21:52:46.39 +72:58:34.7 -- not an asteroid (will add it to exclusion list)
21:53:17.88 +66:04:52.8 -- not an asteroid (will add it to exclusion list)
21:54:34.71 +68:48:26.7 -- not an asteroid (will add it to exclusion list)
21:32:55.57 +69:00:00.2 -- not an asteroid (will add it to exclusion list)
21:29:21.82 +69:58:38.2 -- not an asteroid (will add it to exclusion list)
21:58:03.96 +66:28:13.7 -- not an asteroid (will add it to exclusion list)
20:59:50.59 +71:31:07.3 -- not an asteroid (will add it to exclusion list)
20:55:10.51 +67:02:00.4 -- not an asteroid (will add it to exclusion list)
21:16:14.25 +69:12:27.0 -- not an asteroid (will add it to exclusion list)
21:04:36.71 +68:10:12.0 -- not an asteroid (will add it to exclusion list)
20:35:39.96 +73:00:07.3 -- not an asteroid (will add it to exclusion list)
21:36:28.07 +68:43:42.6 -- not an asteroid (will add it to exclusion list)
21:00:12.28 +66:54:45.3 -- not an asteroid (will add it to exclusion list)
21:31:28.87 +65:35:29.6 -- not an asteroid (will add it to exclusion list)
20:27:55.97 +73:05:42.7 -- not an asteroid (will add it to exclusion list)
22:03:00.53 +71:26:10.2 -- not an asteroid (will add it to exclusion list)
20:22:03.05 +65:25:14.7 -- not an asteroid (will add it to exclusion list)
22:24:58.64 +69:20:32.9 -- not an asteroid (will add it to exclusion list)
21:33:19.56 +65:43:30.0 -- not an asteroid (will add it to exclusion list)
20:57:12.42 +71:42:56.2 -- not an asteroid (will add it to exclusion list)
21:16:46.32 +67:40:14.9 -- not an asteroid (will add it to exclusion list)
21:41:32.29 +67:52:48.4 -- not an asteroid (will add it to exclusion list)
21:51:12.86 +67:56:12.9 -- not an asteroid (will add it to exclusion list)
21:27:49.06 +65:40:02.5 -- not an asteroid (will add it to exclusion list)
21:39:42.82 +65:15:31.9 -- not an asteroid (will add it to exclusion list)
21:08:48.28 +73:26:07.7 -- not an asteroid (will add it to exclusion list)
22:02:06.31 +70:50:22.6 -- not an asteroid (will add it to exclusion list)
21:20:16.23 +71:35:19.6 -- not an asteroid (will add it to exclusion list)
20:03:07.88 +71:38:47.7 -- not an asteroid (will add it to exclusion list)
21:37:17.20 +69:47:52.2 -- not an asteroid (will add it to exclusion list)
22:09:10.23 +70:26:17.9 -- not an asteroid (will add it to exclusion list)
21:18:50.66 +70:28:29.3 -- not an asteroid (will add it to exclusion list)
22:08:26.36 +68:18:10.5 -- not an asteroid (will add it to exclusion list)
22:07:35.53 +67:10:49.1 -- not an asteroid (will add it to exclusion list)
20:06:28.13 +71:56:42.9 -- not an asteroid (will add it to exclusion list)
22:43:06.17 +66:08:59.0 -- not an asteroid (will add it to exclusion list)
21:22:59.08 +68:21:09.7 -- not an asteroid (will add it to exclusion list)
22:21:27.70 +66:26:45.2 -- not an asteroid (will add it to exclusion list)
22:19:51.58 +72:01:25.6 -- not an asteroid (will add it to exclusion list)
21:40:03.24 +70:32:41.7 -- not an asteroid (will add it to exclusion list)
20:56:08.33 +71:33:38.2 -- not an asteroid (will add it to exclusion list)
21:32:12.31 +74:00:38.2 -- not an asteroid (will add it to exclusion list)
21:43:21.59 +68:53:19.2 -- not an asteroid (will add it to exclusion list)
21:47:36.52 +66:28:37.0 -- not an asteroid (will add it to exclusion list)
21:49:51.61 +68:31:23.7 -- not an asteroid (will add it to exclusion list)
22:01:32.82 +70:34:12.3 -- not an asteroid (will add it to exclusion list)
22:20:41.64 +69:23:35.9 -- not an asteroid (will add it to exclusion list)
22:22:18.59 +64:29:43.9 -- not an asteroid (will add it to exclusion list)
21:41:55.66 +70:25:49.3 -- not an asteroid (will add it to exclusion list)
21:57:47.10 +67:04:28.4 -- not an asteroid (will add it to exclusion list)
22:00:26.71 +67:59:46.7 -- not an asteroid (will add it to exclusion list)
22:05:47.84 +73:28:59.3 -- not an asteroid (will add it to exclusion list)
20:48:27.25 +67:05:04.6 -- not an asteroid (will add it to exclusion list)
21:22:03.34 +65:41:36.6 -- not an asteroid (will add it to exclusion list)
21:54:52.97 +72:10:40.9 -- not an asteroid (will add it to exclusion list)
21:04:16.01 +67:42:48.4 -- not an asteroid (will add it to exclusion list)
21:46:14.01 +64:53:57.3 -- not an asteroid (will add it to exclusion list)
21:16:58.14 +72:45:17.3 -- not an asteroid (will add it to exclusion list)
21:41:16.39 +66:40:55.9 -- not an asteroid (will add it to exclusion list)
21:41:39.71 +71:10:04.0 -- not an asteroid (will add it to exclusion list)
21:11:51.02 +65:10:27.7 -- not an asteroid (will add it to exclusion list)
21:53:16.19 +71:49:10.3 -- not an asteroid (will add it to exclusion list)
21:47:55.08 +68:12:32.6 -- not an asteroid (will add it to exclusion list)
22:11:50.28 +70:56:52.3 -- not an asteroid (will add it to exclusion list)
20:35:36.69 +65:09:04.9 -- not an asteroid (will add it to exclusion list)
21:54:36.34 +66:45:26.6 -- not an asteroid (will add it to exclusion list)
21:55:41.98 +67:28:45.3 -- not an asteroid (will add it to exclusion list)
21:29:00.12 +65:39:26.0 -- not an asteroid (will add it to exclusion list)
21:13:19.28 +70:24:05.7 -- not an asteroid (will add it to exclusion list)
21:39:12.14 +68:25:29.0 -- not an asteroid (will add it to exclusion list)
21:55:24.66 +69:11:15.6 -- not an asteroid (will add it to exclusion list)
22:04:31.85 +69:21:23.4 -- not an asteroid (will add it to exclusion list)
21:40:06.91 +69:27:57.8 -- not an asteroid (will add it to exclusion list)
20:55:46.97 +68:12:37.8 -- not an asteroid (will add it to exclusion list)
22:45:07.94 +69:58:34.1 -- not an asteroid (will add it to exclusion list)
21:02:14.59 +70:07:19.3 -- not an asteroid (will add it to exclusion list)
21:07:41.94 +67:34:32.9 -- not an asteroid (will add it to exclusion list)
21:41:47.77 +68:11:38.2 -- not an asteroid (will add it to exclusion list)
21:30:22.78 +70:19:28.3 -- not an asteroid (will add it to exclusion list)
21:52:21.70 +67:18:10.9 -- not an asteroid (will add it to exclusion list)
21:06:45.86 +70:04:20.3 -- not an asteroid (will add it to exclusion list)
22:16:44.98 +66:59:41.9 -- not an asteroid (will add it to exclusion list)
21:25:02.83 +73:15:49.1 -- not an asteroid (will add it to exclusion list)
22:13:23.83 +70:51:08.0 -- not an asteroid (will add it to exclusion list)
21:20:21.40 +68:18:04.2 -- not an asteroid (will add it to exclusion list)
21:36:29.20 +68:33:35.1 -- not an asteroid (will add it to exclusion list)
21:29:10.18 +66:13:07.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:52:59.70 +73:19:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:15.53 +73:23:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:02.31 +73:16:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:32.44 +73:14:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:20.86 +72:45:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:26.86 +73:36:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:54.77 +72:55:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:26.92 +73:21:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:13.12 +73:33:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:16.99 +73:33:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:38.86 +73:28:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:46.26 +73:19:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:16.49 +72:54:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:44.40 +72:06:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:55.27 +72:51:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:41.06 +71:33:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:42.43 +71:34:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:01.33 +72:37:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:01.62 +72:46:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:07.88 +71:38:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:26.43 +70:16:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:28.99 +72:51:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:31.19 +70:29:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:36.79 +70:17:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:44.65 +73:12:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:44.77 +71:36:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:47.27 +71:52:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:23.02 +71:45:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:24.40 +73:03:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:25.34 +73:26:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:29.43 +71:39:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:28.13 +71:56:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:44.38 +69:25:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:32.12 +73:25:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:07.32 +69:37:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:23.34 +72:20:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:02.76 +72:28:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:20.08 +71:09:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:40.38 +70:15:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:46.83 +69:49:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:19.13 +71:52:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:45.72 +71:31:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:51.87 +72:28:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:11.83 +68:43:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:32.15 +72:40:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:32.22 +70:50:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:35.94 +71:38:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:05.12 +68:06:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:27.47 +70:03:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:11.53 +69:46:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:12.43 +69:46:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:27.82 +66:48:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:35.23 +67:18:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:51.72 +68:34:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:41.59 +72:28:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:58.46 +67:19:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:26.15 +73:37:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:40.09 +68:52:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:42.22 +73:49:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:53.53 +73:13:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:53.99 +67:05:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:06.67 +71:38:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:19.83 +66:04:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:23.66 +66:32:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:26.45 +71:38:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:27.23 +69:14:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:29.80 +68:33:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:38.33 +67:00:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:12.08 +69:06:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:13.06 +65:50:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:36.24 +66:09:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:45.45 +70:42:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:55.73 +72:14:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:57.02 +73:41:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:06.58 +71:07:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:11.54 +70:20:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:40.33 +73:44:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:41.24 +71:57:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:45.72 +66:52:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:58.79 +68:45:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:03.05 +65:25:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:25.21 +70:03:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:34.18 +73:11:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:44.01 +65:30:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:54.55 +71:21:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:04.05 +72:42:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:17.51 +71:23:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:23.83 +65:35:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:24.73 +65:42:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:27.96 +66:01:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:34.74 +72:19:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:41.89 +73:45:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:48.88 +73:30:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:50.97 +69:35:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:15.33 +67:12:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:21.08 +64:54:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:48.92 +68:31:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:59.79 +65:11:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:04.46 +72:56:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:26.70 +73:13:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:34.69 +67:29:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:40.31 +64:47:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:41.87 +64:47:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:51.01 +66:05:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:08.99 +67:44:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:21.56 +66:28:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:22.96 +72:03:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:45.80 +67:26:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:47.73 +64:50:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:02.28 +69:55:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:13.43 +65:44:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:14.16 +67:13:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:22.59 +72:44:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:55.97 +73:05:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:28:06.49 +65:41:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:28:21.38 +67:14:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:28:27.06 +74:01:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:28:47.46 +65:52:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:00.01 +73:26:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:02.10 +65:03:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:20.30 +65:10:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:33.52 +67:02:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:08.66 +66:47:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:15.79 +66:44:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:34.81 +65:27:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:45.05 +64:53:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:54.97 +66:38:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:31:21.93 +67:03:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:05.58 +72:59:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:42.06 +68:55:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:53.41 +64:50:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:34:38.76 +66:26:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:35:36.69 +65:09:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:35:39.96 +73:00:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:35:53.84 +74:35:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:36:38.77 +68:17:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:36:46.02 +65:25:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:00.01 +65:15:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:18.22 +64:54:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:14.68 +65:49:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:42.14 +65:29:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:57.00 +68:14:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:11.59 +65:31:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:55.26 +73:32:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:11.29 +65:24:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:39.76 +65:06:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:48.08 +65:27:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:55.67 +65:44:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:09.53 +65:21:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:10.40 +67:20:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:24.26 +65:08:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:40.42 +65:35:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:27.25 +67:05:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:42.41 +72:15:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:53.98 +74:31:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:44.53 +65:12:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:57.19 +65:32:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:48.06 +65:03:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:52.49 +65:53:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:10.51 +67:02:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:46.97 +68:12:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:08.33 +71:33:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:13.48 +73:33:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:12.42 +71:42:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:42.10 +70:03:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:50.59 +71:31:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:06.43 +74:35:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:12.28 +66:54:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:25.44 +71:50:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:07.89 +73:25:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:14.59 +70:07:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:16.01 +67:42:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:26.49 +67:16:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:36.71 +68:10:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:54.54 +67:08:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:06:27.74 +64:59:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:06:45.86 +70:04:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:07:41.94 +67:34:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:08.20 +73:56:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:25.58 +74:43:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:48.28 +73:26:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:51.02 +65:10:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:13.98 +71:03:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:14.44 +71:32:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:19.28 +70:24:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:24.69 +67:59:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:14.25 +69:12:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:17.89 +71:52:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:46.32 +67:40:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:58.14 +72:45:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:58.28 +70:15:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:29.03 +70:30:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:35.63 +70:04:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:15.27 +72:33:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:50.66 +70:28:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:07.36 +65:31:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:16.23 +71:35:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:21.40 +68:18:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:33.74 +73:17:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:37.50 +71:31:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:47.01 +68:08:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:47.91 +71:59:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:03.34 +65:41:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:59.08 +68:21:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:25.12 +69:08:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:02.83 +73:15:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:27.43 +69:56:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:54.18 +70:13:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:31.45 +71:48:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:46.01 +65:10:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:49.06 +65:40:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:06.02 +66:20:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:00.12 +65:39:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:10.18 +66:13:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:21.82 +69:58:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:22.78 +70:19:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.87 +65:35:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:02.72 +65:09:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:05.49 +68:03:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:12.31 +74:00:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:55.57 +69:00:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:19.56 +65:43:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:24.17 +66:57:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:42.56 +68:39:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:28.07 +68:43:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:29.20 +68:33:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:17.20 +69:47:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:38.29 +73:03:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:44.92 +70:56:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:09.36 +73:29:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:10.31 +68:16:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:12.14 +68:25:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:14.96 +65:43:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:25.53 +67:58:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:33.81 +69:28:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:42.82 +65:15:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:03.24 +70:32:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:06.91 +69:27:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:08.63 +68:02:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:30.50 +66:26:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:31.74 +74:08:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:16.39 +66:40:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:32.29 +67:52:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:39.71 +71:10:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:44.97 +66:52:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:47.77 +68:11:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:55.66 +70:25:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:52.00 +69:55:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:21.59 +68:53:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:03.52 +66:39:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:42.07 +67:49:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:28.22 +66:00:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:12.20 +67:38:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:14.01 +64:53:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:22.69 +69:11:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:37.15 +67:13:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:36.52 +66:28:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:45.12 +72:57:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:55.08 +68:12:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:28.57 +67:49:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:42.03 +68:15:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:51.61 +68:31:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:30.84 +69:17:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:12.86 +67:56:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:16.86 +71:04:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:21.70 +67:18:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:46.39 +72:58:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:52.86 +69:03:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:16.19 +71:49:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:17.88 +66:04:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:46.05 +69:03:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:34.71 +68:48:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:36.34 +66:45:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:52.97 +72:10:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:53.46 +69:42:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:24.66 +69:11:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:34.44 +67:08:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:41.98 +67:28:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:33.79 +71:18:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:34.51 +65:02:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:47.10 +67:04:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:48.17 +67:56:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:03.96 +66:28:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:22.06 +65:57:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:26.71 +67:59:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:42.55 +70:37:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:43.17 +65:03:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:32.82 +70:34:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:06.31 +70:50:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:00.53 +71:26:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:31.85 +69:21:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:23.09 +64:41:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:47.84 +73:28:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:11.90 +72:02:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:23.95 +69:04:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:35.06 +70:08:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:35.53 +67:10:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:26.36 +68:18:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:10.23 +70:26:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:49.30 +70:18:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:50.28 +70:56:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:23.83 +70:51:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:54.07 +65:06:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:44.98 +66:59:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:51.58 +72:01:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:41.64 +69:23:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:27.70 +66:26:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:18.59 +64:29:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:58.64 +69:20:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:55.72 +68:25:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:31:29.97 +67:23:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:32:12.21 +67:18:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:32:58.85 +66:54:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:34:35.47 +69:06:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:35:41.14 +64:40:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:40:35.93 +66:30:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:43:06.17 +66:08:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:45:07.94 +69:58:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:46:00.15 +67:07:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:55:56.82 +67:20:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:10.28 +70:02:27.3 -- 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)
19:52:59.70 +73:19:19.9 -- not a known variable star
19:54:15.53 +73:23:22.0 -- not a known variable star
19:55:02.31 +73:16:00.1 -- not a known variable star
19:55:32.44 +73:14:48.3 -- not a known variable star
19:56:20.86 +72:45:39.5 -- not a known variable star
19:56:26.86 +73:36:58.5 -- a known variable star
19:56:54.77 +72:55:15.2 -- not a known variable star
19:57:26.92 +73:21:20.6 -- not a known variable star
19:59:13.12 +73:33:35.1 -- not a known variable star
19:59:16.99 +73:33:21.4 -- not a known variable star
19:59:38.86 +73:28:15.3 -- not a known variable star
19:59:46.26 +73:19:43.4 -- not a known variable star
20:01:16.49 +72:54:15.9 -- not a known variable star
20:01:44.40 +72:06:09.3 -- a known variable star
20:01:55.27 +72:51:00.7 -- not a known variable star
20:02:41.06 +71:33:47.3 -- not a known variable star
20:02:42.43 +71:34:15.7 -- not a known variable star
20:03:01.33 +72:37:10.6 -- not a known variable star
20:03:01.62 +72:46:36.9 -- not a known variable star
20:03:07.88 +71:38:47.7 -- not a known variable star
20:03:26.43 +70:16:18.6 -- not a known variable star
20:03:28.99 +72:51:43.8 -- not a known variable star
20:03:31.19 +70:29:17.7 -- not a known variable star
20:03:36.79 +70:17:56.0 -- a known variable star
20:03:44.65 +73:12:47.0 -- not a known variable star
20:03:44.77 +71:36:25.5 -- not a known variable star
20:03:47.27 +71:52:53.9 -- not a known variable star
20:04:23.02 +71:45:46.6 -- not a known variable star
20:04:24.40 +73:03:41.1 -- not a known variable star
20:05:25.34 +73:26:03.6 -- not a known variable star
20:05:29.43 +71:39:22.0 -- not a known variable star
20:06:28.13 +71:56:42.9 -- not a known variable star
20:07:44.38 +69:25:31.1 -- not a known variable star
20:09:32.12 +73:25:53.3 -- not a known variable star
20:10:07.32 +69:37:48.8 -- not a known variable star
20:10:23.34 +72:20:54.4 -- not a known variable star
20:12:02.76 +72:28:59.7 -- not a known variable star
20:12:20.08 +71:09:34.7 -- not a known variable star
20:12:40.38 +70:15:02.5 -- not a known variable star
20:12:46.83 +69:49:54.9 -- not a known variable star
20:13:19.13 +71:52:00.7 -- not a known variable star
20:13:45.72 +71:31:44.4 -- not a known variable star
20:13:51.87 +72:28:28.7 -- not a known variable star
20:14:11.83 +68:43:31.7 -- not a known variable star
20:14:32.15 +72:40:17.3 -- not a known variable star
20:14:32.22 +70:50:20.6 -- not a known variable star
20:14:35.94 +71:38:05.2 -- not a known variable star
20:15:05.12 +68:06:40.0 -- a known variable star
20:15:27.47 +70:03:17.2 -- not a known variable star
20:16:11.53 +69:46:08.0 -- not a known variable star
20:16:12.43 +69:46:10.5 -- not a known variable star
20:16:27.82 +66:48:30.4 -- not a known variable star
20:16:35.23 +67:18:38.9 -- not a known variable star
20:16:51.72 +68:34:54.6 -- not a known variable star
20:17:41.59 +72:28:52.0 -- not a known variable star
20:17:58.46 +67:19:00.6 -- not a known variable star
20:18:26.15 +73:37:09.6 -- not a known variable star
20:18:40.09 +68:52:26.1 -- not a known variable star
20:18:42.22 +73:49:31.7 -- not a known variable star
20:18:53.53 +73:13:04.2 -- not a known variable star
20:18:53.99 +67:05:18.8 -- not a known variable star
20:19:06.67 +71:38:51.7 -- not a known variable star
20:19:19.83 +66:04:25.8 -- not a known variable star
20:19:23.66 +66:32:14.4 -- not a known variable star
20:19:26.45 +71:38:05.7 -- not a known variable star
20:19:27.23 +69:14:32.4 -- a known variable star
20:19:29.80 +68:33:12.6 -- not a known variable star
20:19:38.33 +67:00:13.0 -- not a known variable star
20:20:12.08 +69:06:04.5 -- not a known variable star
20:20:13.06 +65:50:49.1 -- a known variable star
20:20:36.24 +66:09:01.0 -- not a known variable star
20:20:45.45 +70:42:26.9 -- not a known variable star
20:20:55.73 +72:14:23.8 -- not a known variable star
20:20:57.02 +73:41:09.9 -- not a known variable star
20:21:06.58 +71:07:52.6 -- not a known variable star
20:21:11.54 +70:20:32.7 -- not a known variable star
20:21:40.33 +73:44:41.2 -- not a known variable star
20:21:41.24 +71:57:48.9 -- not a known variable star
20:21:45.72 +66:52:05.8 -- not a known variable star
20:21:58.79 +68:45:18.2 -- not a known variable star
20:22:03.05 +65:25:14.7 -- a known variable star
20:22:25.21 +70:03:41.4 -- not a known variable star
20:22:34.18 +73:11:29.5 -- not a known variable star
20:22:44.01 +65:30:16.7 -- not a known variable star
20:22:54.55 +71:21:28.8 -- not a known variable star
20:23:04.05 +72:42:26.1 -- not a known variable star
20:23:17.51 +71:23:23.0 -- not a known variable star
20:23:23.83 +65:35:13.5 -- not a known variable star
20:23:24.73 +65:42:34.7 -- not a known variable star
20:23:27.96 +66:01:10.9 -- not a known variable star
20:23:34.74 +72:19:48.6 -- not a known variable star
20:23:41.89 +73:45:15.7 -- not a known variable star
20:23:48.88 +73:30:27.0 -- not a known variable star
20:23:50.97 +69:35:48.2 -- a known variable star
20:24:15.33 +67:12:31.1 -- not a known variable star
20:24:21.08 +64:54:57.6 -- not a known variable star
20:24:48.92 +68:31:58.8 -- not a known variable star
20:24:59.79 +65:11:28.0 -- a known variable star
20:25:04.46 +72:56:16.7 -- not a known variable star
20:25:26.70 +73:13:53.6 -- not a known variable star
20:25:34.69 +67:29:45.2 -- not a known variable star
20:25:40.31 +64:47:48.0 -- not a known variable star
20:25:41.87 +64:47:58.4 -- not a known variable star
20:25:51.01 +66:05:13.4 -- not a known variable star
20:26:08.99 +67:44:09.2 -- not a known variable star
20:26:21.56 +66:28:43.2 -- not a known variable star
20:26:22.96 +72:03:22.8 -- a known variable star
20:26:45.80 +67:26:55.8 -- not a known variable star
20:26:47.73 +64:50:46.9 -- a known variable star
20:27:02.28 +69:55:32.6 -- not a known variable star
20:27:13.43 +65:44:51.3 -- not a known variable star
20:27:14.16 +67:13:17.7 -- not a known variable star
20:27:22.59 +72:44:39.6 -- not a known variable star
20:27:55.97 +73:05:42.7 -- a known variable star
20:28:06.49 +65:41:43.7 -- not a known variable star
20:28:21.38 +67:14:59.5 -- a known variable star
20:28:27.06 +74:01:30.0 -- not a known variable star
20:28:47.46 +65:52:11.8 -- not a known variable star
20:29:00.01 +73:26:37.9 -- not a known variable star
20:29:02.10 +65:03:54.2 -- not a known variable star
20:29:20.30 +65:10:13.0 -- not a known variable star
20:29:33.52 +67:02:15.7 -- a known variable star
20:30:08.66 +66:47:01.5 -- not a known variable star
20:30:15.79 +66:44:12.1 -- not a known variable star
20:30:34.81 +65:27:11.2 -- not a known variable star
20:30:45.05 +64:53:06.6 -- not a known variable star
20:30:54.97 +66:38:55.6 -- not a known variable star
20:31:21.93 +67:03:47.4 -- not a known variable star
20:32:05.58 +72:59:00.9 -- not a known variable star
20:32:42.06 +68:55:05.8 -- a known variable star
20:32:53.41 +64:50:36.0 -- not a known variable star
20:34:38.76 +66:26:22.1 -- not a known variable star
20:35:36.69 +65:09:04.9 -- not a known variable star
20:35:39.96 +73:00:07.3 -- a known variable star
20:35:53.84 +74:35:02.3 -- not a known variable star
20:36:38.77 +68:17:39.4 -- a known variable star
20:36:46.02 +65:25:39.3 -- not a known variable star
20:37:00.01 +65:15:24.6 -- a known variable star
20:37:18.22 +64:54:39.8 -- a known variable star
20:38:14.68 +65:49:47.4 -- a known variable star
20:38:42.14 +65:29:22.4 -- not a known variable star
20:38:57.00 +68:14:26.9 -- not a known variable star
20:39:11.59 +65:31:13.9 -- not a known variable star
20:39:55.26 +73:32:07.8 -- not a known variable star
20:41:11.29 +65:24:06.7 -- not a known variable star
20:41:39.76 +65:06:35.0 -- a known variable star
20:41:48.08 +65:27:05.6 -- not a known variable star
20:41:55.67 +65:44:21.6 -- a known variable star
20:43:09.53 +65:21:09.8 -- not a known variable star
20:44:10.40 +67:20:30.7 -- a known variable star
20:44:24.26 +65:08:24.0 -- a known variable star
20:44:40.42 +65:35:08.2 -- not a known variable star
20:48:27.25 +67:05:04.6 -- a known variable star
20:49:42.41 +72:15:49.0 -- a known variable star
20:49:53.98 +74:31:35.6 -- a known variable star
20:51:44.53 +65:12:30.1 -- not a known variable star
20:53:57.19 +65:32:08.1 -- not a known variable star
20:54:48.06 +65:03:49.9 -- not a known variable star
20:54:52.49 +65:53:47.2 -- not a known variable star
20:55:10.51 +67:02:00.4 -- a known variable star
20:55:46.97 +68:12:37.8 -- a known variable star
20:56:08.33 +71:33:38.2 -- a known variable star
20:56:13.48 +73:33:30.4 -- a known variable star
20:57:12.42 +71:42:56.2 -- a known variable star
20:58:42.10 +70:03:25.5 -- a known variable star
20:59:50.59 +71:31:07.3 -- a known variable star
21:00:06.43 +74:35:21.9 -- a known variable star
21:00:12.28 +66:54:45.3 -- a known variable star
21:00:25.44 +71:50:23.1 -- a known variable star
21:02:07.89 +73:25:45.2 -- a known variable star
21:02:14.59 +70:07:19.3 -- a known variable star
21:04:16.01 +67:42:48.4 -- a known variable star
21:04:26.49 +67:16:07.2 -- a known variable star
21:04:36.71 +68:10:12.0 -- a known variable star
21:04:54.54 +67:08:11.9 -- a known variable star
21:06:27.74 +64:59:50.8 -- a known variable star
21:06:45.86 +70:04:20.3 -- a known variable star
21:07:41.94 +67:34:32.9 -- a known variable star
21:08:08.20 +73:56:04.0 -- a known variable star
21:08:25.58 +74:43:29.6 -- a known variable star
21:08:48.28 +73:26:07.7 -- a known variable star
21:11:51.02 +65:10:27.7 -- not a known variable star
21:12:13.98 +71:03:50.3 -- a known variable star
21:12:14.44 +71:32:36.7 -- a known variable star
21:13:19.28 +70:24:05.7 -- a known variable star
21:14:24.69 +67:59:10.0 -- a known variable star
21:16:14.25 +69:12:27.0 -- a known variable star
21:16:17.89 +71:52:09.3 -- a known variable star
21:16:46.32 +67:40:14.9 -- a known variable star
21:16:58.14 +72:45:17.3 -- a known variable star
21:16:58.28 +70:15:44.2 -- a known variable star
21:17:29.03 +70:30:50.9 -- a known variable star
21:17:35.63 +70:04:34.1 -- not a known variable star
21:18:15.27 +72:33:05.5 -- a known variable star
21:18:50.66 +70:28:29.3 -- a known variable star
21:19:07.36 +65:31:18.3 -- a known variable star
21:20:16.23 +71:35:19.6 -- a known variable star
21:20:21.40 +68:18:04.2 -- a known variable star
21:20:33.74 +73:17:58.7 -- a known variable star
21:20:37.50 +71:31:11.0 -- a known variable star
21:20:47.01 +68:08:38.4 -- not a known variable star
21:20:47.91 +71:59:54.6 -- a known variable star
21:22:03.34 +65:41:36.6 -- not a known variable star
21:22:59.08 +68:21:09.7 -- a known variable star
21:23:25.12 +69:08:59.2 -- a known variable star
21:25:02.83 +73:15:49.1 -- a known variable star
21:26:27.43 +69:56:56.6 -- a known variable star
21:26:54.18 +70:13:15.4 -- a known variable star
21:27:31.45 +71:48:57.4 -- a known variable star
21:27:46.01 +65:10:07.8 -- not a known variable star
21:27:49.06 +65:40:02.5 -- a known variable star
21:28:06.02 +66:20:29.5 -- a known variable star
21:29:00.12 +65:39:26.0 -- a known variable star
21:29:10.18 +66:13:07.9 -- a known variable star
21:29:21.82 +69:58:38.2 -- a known variable star
21:30:22.78 +70:19:28.3 -- a known variable star
21:31:28.87 +65:35:29.6 -- a known variable star
21:32:02.72 +65:09:50.2 -- a known variable star
21:32:05.49 +68:03:34.6 -- not a known variable star
21:32:12.31 +74:00:38.2 -- a known variable star
21:32:55.57 +69:00:00.2 -- a known variable star
21:33:19.56 +65:43:30.0 -- a known variable star
21:33:24.17 +66:57:46.7 -- a known variable star
21:35:42.56 +68:39:08.6 -- a known variable star
21:36:28.07 +68:43:42.6 -- a known variable star
21:36:29.20 +68:33:35.1 -- not a known variable star
21:37:17.20 +69:47:52.2 -- a known variable star
21:38:38.29 +73:03:03.8 -- a known variable star
21:38:44.92 +70:56:59.3 -- not a known variable star
21:39:09.36 +73:29:25.4 -- a known variable star
21:39:10.31 +68:16:13.8 -- a known variable star
21:39:12.14 +68:25:29.0 -- a known variable star
21:39:14.96 +65:43:35.8 -- a known variable star
21:39:25.53 +67:58:26.2 -- a known variable star
21:39:33.81 +69:28:37.5 -- a known variable star
21:39:42.82 +65:15:31.9 -- a known variable star
21:40:03.24 +70:32:41.7 -- a known variable star
21:40:06.91 +69:27:57.8 -- a known variable star
21:40:08.63 +68:02:45.2 -- a known variable star
21:40:30.50 +66:26:04.9 -- a known variable star
21:40:31.74 +74:08:03.4 -- a known variable star
21:41:16.39 +66:40:55.9 -- a known variable star
21:41:32.29 +67:52:48.4 -- a known variable star
21:41:39.71 +71:10:04.0 -- a known variable star
21:41:44.97 +66:52:46.6 -- a known variable star
21:41:47.77 +68:11:38.2 -- not a known variable star
21:41:55.66 +70:25:49.3 -- a known variable star
21:42:52.00 +69:55:15.2 -- a known variable star
21:43:21.59 +68:53:19.2 -- a known variable star
21:44:03.52 +66:39:14.1 -- a known variable star
21:44:42.07 +67:49:31.0 -- a known variable star
21:45:28.22 +66:00:19.7 -- a known variable star
21:46:12.20 +67:38:13.5 -- a known variable star
21:46:14.01 +64:53:57.3 -- a known variable star
21:46:22.69 +69:11:06.8 -- a known variable star
21:46:37.15 +67:13:12.6 -- a known variable star
21:47:36.52 +66:28:37.0 -- a known variable star
21:47:45.12 +72:57:46.7 -- a known variable star
21:47:55.08 +68:12:32.6 -- a known variable star
21:48:28.57 +67:49:45.4 -- not a known variable star
21:48:42.03 +68:15:09.6 -- not a known variable star
21:49:51.61 +68:31:23.7 -- a known variable star
21:50:30.84 +69:17:46.9 -- a known variable star
21:51:12.86 +67:56:12.9 -- a known variable star
21:51:16.86 +71:04:29.5 -- not a known variable star
21:52:21.70 +67:18:10.9 -- a known variable star
21:52:46.39 +72:58:34.7 -- a known variable star
21:52:52.86 +69:03:51.1 -- a known variable star
21:53:16.19 +71:49:10.3 -- a known variable star
21:53:17.88 +66:04:52.8 -- a known variable star
21:53:46.05 +69:03:54.2 -- not a known variable star
21:54:34.71 +68:48:26.7 -- a known variable star
21:54:36.34 +66:45:26.6 -- a known variable star
21:54:52.97 +72:10:40.9 -- a known variable star
21:54:53.46 +69:42:29.0 -- not a known variable star
21:55:24.66 +69:11:15.6 -- a known variable star
21:55:34.44 +67:08:08.4 -- a known variable star
21:55:41.98 +67:28:45.3 -- a known variable star
21:57:33.79 +71:18:24.7 -- a known variable star
21:57:34.51 +65:02:12.5 -- a known variable star
21:57:47.10 +67:04:28.4 -- a known variable star
21:57:48.17 +67:56:56.6 -- a known variable star
21:58:03.96 +66:28:13.7 -- a known variable star
21:58:22.06 +65:57:05.5 -- a known variable star
22:00:26.71 +67:59:46.7 -- a known variable star
22:00:42.55 +70:37:56.1 -- a known variable star
22:00:43.17 +65:03:51.0 -- a known variable star
22:01:32.82 +70:34:12.3 -- a known variable star
22:02:06.31 +70:50:22.6 -- not a known variable star
22:03:00.53 +71:26:10.2 -- a known variable star
22:04:31.85 +69:21:23.4 -- a known variable star
22:05:23.09 +64:41:46.0 -- a known variable star
22:05:47.84 +73:28:59.3 -- a known variable star
22:06:11.90 +72:02:18.3 -- a known variable star
22:07:23.95 +69:04:10.5 -- not a known variable star
22:07:35.06 +70:08:20.1 -- a known variable star
22:07:35.53 +67:10:49.1 -- a known variable star
22:08:26.36 +68:18:10.5 -- a known variable star
22:09:10.23 +70:26:17.9 -- not a known variable star
22:09:49.30 +70:18:31.1 -- a known variable star
22:11:50.28 +70:56:52.3 -- a known variable star
22:13:23.83 +70:51:08.0 -- not a known variable star
22:15:54.07 +65:06:37.1 -- a known variable star
22:16:44.98 +66:59:41.9 -- a known variable star
22:19:51.58 +72:01:25.6 -- a known variable star
22:20:41.64 +69:23:35.9 -- not a known variable star
22:21:27.70 +66:26:45.2 -- a known variable star
22:22:18.59 +64:29:43.9 -- a known variable star
22:24:58.64 +69:20:32.9 -- a known variable star
22:26:55.72 +68:25:12.9 -- a known variable star
22:31:29.97 +67:23:50.0 -- a known variable star
22:32:12.21 +67:18:10.0 -- a known variable star
22:32:58.85 +66:54:43.5 -- a known variable star
22:34:35.47 +69:06:22.7 -- a known variable star
22:35:41.14 +64:40:01.7 -- a known variable star
22:40:35.93 +66:30:39.0 -- a known variable star
22:43:06.17 +66:08:59.0 -- a known variable star
22:45:07.94 +69:58:34.1 -- a known variable star
22:46:00.15 +67:07:22.6 -- a known variable star
22:55:56.82 +67:20:39.8 -- a known variable star
23:00:10.28 +70:02:27.3 -- a known variable star
Found 151 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
321 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
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.64852988 -observatory 500
23:23:23.72 -01:59:26.2 Mercury (-0.1mag)
23:04:22.50 -07:30:23.6 Venus (-3.9mag)
21:42:45.16 -14:53:08.4 Mars (1.1mag)
07:06:06.29 +22:54:19.5 Jupiter (-2.5mag)
00:05:25.69 -01:44:31.3 Saturn (1.0mag)
03:39:59.42 +19:21:43.4 Uranus (5.7mag)
00:03:40.75 -01:01:38.3 Neptune (7.8mag)
20:29:06.91 -22:59:34.5 Pluto (14.5mag)
01:53:13.33 +16:08:46.9 Moon (-9.6mag)
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.64852988:
07:06:10.19 +22:54:14.5 Io (5.4mag)
07:06:17.71 +22:53:58.6 Europa (5.5mag)
07:05:56.90 +22:54:45.4 Ganymede (4.9mag)
07:06:25.21 +22:53:54.3 Callisto (6.2mag)
07:09:15.20 +23:10:42.8 Himalia (15.0mag)
07:06:07.39 +22:54:19.8 Thebe (15.9mag)
07:08:40.28 +23:19:11.0 Elara (17.0mag)
07:01:39.80 +24:02:18.2 Pasiphae (17.0mag)
07:15:07.19 +22:42:19.3 Carme (18.1mag)
00:05:37.38 -01:44:35.9 Titan (8.8mag)
00:05:31.14 -01:44:30.0 Rhea (10.1mag)
00:05:21.06 -01:45:52.3 Iapetus (11.5mag)
00:05:26.49 -01:44:34.4 Hyperion (14.8mag)
00:07:29.97 -01:31:31.2 Phoebe (16.8mag)
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.64852988:
08:45:44.17 +24:30:42.5 JWST
11:29:35.07 +47:59:53.8 Chandra
15:19:45.37 -60:03:10.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 01:32 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)2461093.64852988 at 500
16:59:40.93 -11:03:49.0 17.5mag 10P/Tempel 2
03:37:18.40 +28:57:48.1 18.0mag 123P/West-Hartley
08:23:39.32 +60:43:00.7 18.4mag 124P/Mrkos
21:19:33.42 -07:38:53.1 22.1mag 141P/Machholz
01:21:08.15 +11:54:44.9 17.7mag 145P/Shoemaker-Levy 5
11:02:59.37 +30:34:29.8 17.9mag 164P/Christensen
04:45:17.19 +19:20:56.7 0.0mag 195P/Hill
15:52:03.27 -06:35:55.1 19.2mag 210P/Christensen
18:16:49.78 -21:28:32.0 17.3mag 218P/LINEAR
16:21:33.54 -18:10:56.8 15.2mag 235P/LINEAR
03:56:22.85 +27:44:26.8 17.8mag 240P/NEAT
15:17:37.38 +06:38:26.6 14.8mag 24P/Schaumasse
11:23:31.22 -03:23:10.2 17.4mag 29P/Schwassmann-Wachmann 1
04:45:17.19 +19:20:56.7 0.0mag 407P/PanSTARRS-Fuls
17:07:08.17 -11:19:14.4 17.6mag 40P/Vaisala 1
11:02:13.09 -08:51:54.1 16.6mag 43P/Wolf-Harrington
13:25:29.72 -05:49:38.1 20.0mag 489P/Denning
04:34:21.85 +48:34:35.6 17.8mag 493P/2024 Q2 (LONEOS)
06:04:23.04 +47:31:31.4 17.7mag 63P/Wild 1
23:14:35.84 -02:07:34.6 16.2mag 78P/Gehrels 2
20:01:29.03 -22:18:21.0 15.0mag 88P/Howell
15:27:54.50 -29:00:39.3 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.08 -72:35:55.4 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:50.03 +31:12:54.1 18.2mag C/2017 K2 (PanSTARRS)
20:06:38.08 -65:11:37.6 18.1mag C/2020 V2 (ZTF)
17:21:40.28 +04:21:21.1 16.3mag C/2021 G2 (ATLAS)
03:35:40.77 +24:36:41.9 15.8mag C/2022 N2 (PanSTARRS)
09:08:13.35 +29:49:33.1 15.3mag C/2022 QE78 (ATLAS)
08:35:40.64 -06:33:49.1 16.7mag C/2022 R6 (PanSTARRS)
23:53:01.81 +48:26:44.8 18.0mag C/2023 C2 (ATLAS)
09:51:08.14 -20:46:01.6 17.5mag C/2023 F3 (ATLAS)
20:34:44.74 +61:14:30.9 17.3mag C/2023 H5 (Lemmon)
19:34:30.10 -03:24:15.8 16.1mag C/2023 R1 (PANSTARRS)
02:48:55.19 +35:40:34.4 18.5mag C/2023 RS61 (PanSTARRS)
21:01:26.62 +81:19:56.2 18.0mag C/2023 X2 (Lemmon)
06:39:10.13 +63:49:13.0 17.3mag C/2024 A1 (ATLAS)
01:56:43.41 -24:38:10.5 11.2mag C/2024 E1 (Wierzchos)
11:44:58.89 -02:34:53.8 18.1mag C/2024 G2 (ATLAS)
19:28:18.75 +00:39:12.1 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.74 -01:42:54.7 17.7mag C/2024 G6 (ATLAS)
19:53:27.42 +03:15:04.2 15.6mag C/2024 J3 (ATLAS)
02:47:14.47 -31:34:31.5 15.4mag C/2024 T5 (ATLAS)
16:25:06.70 -58:13:43.3 15.6mag C/2025 A6 (Lemmon)
04:50:29.54 +62:14:36.3 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)
15:56:43.60 -13:01:27.9 14.8mag C/2025 L1 (ATLAS)
02:20:13.88 -19:05:56.2 16.7mag C/2025 Q3 (ATLAS)
02:09:34.22 +17:16:42.8 21.2mag C/2025 R2 (SWAN)
22:20:45.78 +17:39:14.3 16.4mag C/2025 R3 (PANSTARRS)
21:46:01.01 -16:50:22.3 21.5mag C/2025 T1 (ATLAS)
03:06:14.94 -20:34:08.2 18.3mag C/2026 A1 (MAPS)
21:03:01.14 +20:55:31.9 16.9mag C/2026 B2 (Sun-Gao)
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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
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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 22 01:32 tocp_transients_list.txt